<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JAMP</journal-id><journal-title-group><journal-title>Journal of Applied Mathematics and Physics</journal-title></journal-title-group><issn pub-type="epub">2327-4352</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jamp.2014.28092</article-id><article-id pub-id-type="publisher-id">JAMP-47947</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>PHYSICS &amp; MATHEMATICS</subject></subj-group></article-categories><title-group><article-title>Curvature Motion on Dual Hyperbolic Unit Sphere H<sup>2</sup><sub style="margin-left:-8px;">0</sub></article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ziya</surname><given-names>Yapar</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yasemin</surname><given-names>Sağıroğlu</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Karadeniz Technical University, Trabzon, Turkey</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>sagiroglu.yasemin@gmail.com(YS)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>27</day><month>06</month><year>2014</year></pub-date><volume>02</volume><issue>08</issue><fpage>828</fpage><lpage>836</lpage><history><date date-type="received"><day>1</day>	<month>June</month>	<year>2014</year></date><date date-type="rev-recd"><day>1</day>	<month>July</month>	<year>2014</year>	</date><date date-type="accepted"><day>13</day>	<month>July</month>	<year>2014</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
	In this paper, we define
dual curvature motion on the dual hyperbolic unit sphere H&lt;sup&gt;2&lt;/sup&gt;&lt;sub
style="margin-left:-8px;"&gt;0&lt;/sub&gt; in the dual Lorentzian
space D&lt;sup&gt;3&lt;/sup&gt;&lt;sub style="margin-left:-8px;"&gt;1&lt;/sub&gt;
with dual signature (+,+-) . We carry the obtained
results to the Lorentzian line space R&lt;sup&gt;3&lt;/sup&gt;&lt;sub
style="margin-left:-8px;"&gt;1&lt;/sub&gt; by means of Study mapping.
Then we make an analysis of the orbits during the dual hyperbolic spherical
curvature motion. Finally, we find some line congruences, the family of ruled
surfaces and ruled surfaces in R&lt;sup&gt;3&lt;/sup&gt;&lt;sub
style="margin-left:-8px;"&gt;1&lt;/sub&gt;.

</p></abstract><kwd-group><kwd>Dual Curvature Motion</kwd><kwd> Dual Lorentzian Space</kwd><kwd> Study Mapping</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Dual numbers had been introduced by W.K. Clifford (1845-1849) as a tool for his geometrical investigations. After him, E. Study (1860-1930) used dual numbers and dual vectors in his research on the geometry of lines and kinematics [<xref ref-type="bibr" rid="scirp.47947-ref1">1</xref>] . He devoted special attention to the representation of directed lines by dual unit vectors and defined the mapping that is known by his name. There exists one-to-one correspondence between the vectors of dual unit sphere <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8ebcd98c-7239-4285-8294-b3f51b5cd29f.png" xlink:type="simple"/></inline-formula> and the directed lines of space of lines<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e3582c65-87fa-4b54-a061-b73cb393bb7a.png" xlink:type="simple"/></inline-formula>. Hence, a differentiable curve on the sphere <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\a94e0216-de94-4a23-99f8-a2ab43256b7c.png" xlink:type="simple"/></inline-formula> corresponds to a ruled surface in the line space <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3a5d999a-70c9-481d-91e6-aa3a3b9b6340.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.47947-ref2">2</xref>] -[<xref ref-type="bibr" rid="scirp.47947-ref4">4</xref>] . Ruled surfaces have been widely applied in surface design, manufacturing technology and simulation of rigid bodies [<xref ref-type="bibr" rid="scirp.47947-ref5">5</xref>] .</p><p>E. Study’s mapping plays a fundamental role in the real and dual Lorentzian spaces [<xref ref-type="bibr" rid="scirp.47947-ref6">6</xref>] . By this mapping, a curve on a dual hyperbolic unit sphere <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0402e07a-7ab0-4c90-ac32-dfdfb6ec1124.png" xlink:type="simple"/></inline-formula> corresponds to a timelike ruled surface in the Lorentzian line space<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0e4af728-3fc1-4481-80a7-3e69b2cf4a0d.png" xlink:type="simple"/></inline-formula>, in other words, there exists a one-to-one correspondence between the geometry of curves on <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\87853bf0-253e-4ce0-8d7e-a8139e82c649.png" xlink:type="simple"/></inline-formula> and the geometry of timelike ruled surfaces in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\46c3fabc-07e0-4fbf-9720-a914f9278196.png" xlink:type="simple"/></inline-formula>. Similarly, a timelike (spacelike) curve on a dual Lorentzian unit sphere <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7838699d-7f70-4e81-bada-71100f2b161d.png" xlink:type="simple"/></inline-formula> corresponds to a spacelike (timelike) ruled surface in the Lorentzian line space<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\03d11ff8-1bf9-4a62-b4cf-9bf9f5426696.png" xlink:type="simple"/></inline-formula>, this means that, there exists a one-to-one correspondence between the geometry of timelike (spacelike) curves on <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d65f7832-0fb9-4d8b-a8a0-9364f3dced04.png" xlink:type="simple"/></inline-formula> and the geometry of spacelike (timelike) ruled surfaces in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4b3264e6-4104-46f7-bb22-302a3542310d.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.47947-ref7">7</xref>] . Since the dual Lorentzian metric is indefinite, the angle concept in this space is very interesting. For instance, the dual hyperbolic angle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4a376a2a-b27e-48cf-a804-11f7513f51e5.png" xlink:type="simple"/></inline-formula> between two dual timelike unit vectors is a dual value formed with the (real) hyperbolic angle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\5ca9ce17-f0ca-492e-a020-6ff2a096838b.png" xlink:type="simple"/></inline-formula> between corresponding two directed timelike lines in the Lorentzian line space <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\49f2d8d5-84f8-4429-936e-a37d704486db.png" xlink:type="simple"/></inline-formula> and the shortest Lorentzian distance <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e5986ba7-e28b-44d7-be75-1bc6e6ed8a73.png" xlink:type="simple"/></inline-formula> between these directed timelike lines.</p><p>Real spherical curvature motion had been introduced by A. Karger and J. Novak [<xref ref-type="bibr" rid="scirp.47947-ref8">8</xref>] . Also, a dual spherical curvature motion has been defined by Z. Yapar [<xref ref-type="bibr" rid="scirp.47947-ref9">9</xref>] . In recent years, study about the real spherical motion has been generalized to the Lorentz spherical motion [<xref ref-type="bibr" rid="scirp.47947-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.47947-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.47947-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.47947-ref11">11</xref>] . In this work, we consider the curvature motion on the dual hyperbolic unit sphere <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\61036252-479f-486f-827a-adf585eb07b9.png" xlink:type="simple"/></inline-formula> of the dual Lorentzian space <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\be2c38f2-939e-4484-8542-e4b2fe00beba.png" xlink:type="simple"/></inline-formula> and the results are carried over to the Lorentzian line space by the E. Study’s mapping.</p></sec><sec id="s2"><title>2. Preliminaries and Definitions</title><p>In this section, we give a brief summary of the theory of dual numbers, dual Lorentzian vectors and Study’s mapping.</p><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4450cbc1-9733-4439-b20a-6a51227945c9.png" xlink:type="simple"/></inline-formula> be the 3-dimensional Minkowski space over the field of real numbers <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\29b18344-d302-413f-92a6-624e23500f14.png" xlink:type="simple"/></inline-formula> with the Lorentzian inner product <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e0ae9fe5-4111-4a30-954c-b632da318a1c.png" xlink:type="simple"/></inline-formula> given by</p><disp-formula id="scirp.47947-formula3348"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\840c8199-641a-4d34-acba-003a8cd2da63.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8edb1b57-7e07-4a59-bd97-539a48879e6b.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\beb5d869-e45f-404a-bcac-b5699a433da0.png" xlink:type="simple"/></inline-formula>.</p><p>A vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d875407d-af75-43a5-a0c3-09bf9a57e99f.png" xlink:type="simple"/></inline-formula> of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6c90b110-8db2-4ed1-a99a-9800defc8cbd.png" xlink:type="simple"/></inline-formula> is said to be timelikeif<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6c49ff45-196b-45c0-ab90-5cc32c7bd610.png" xlink:type="simple"/></inline-formula>, spacelike if <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e2005354-d28e-482a-aa65-894160ccfaf3.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\89c306d0-2fc9-4e5d-ae97-b4e312e08a65.png" xlink:type="simple"/></inline-formula>, and lighlike (null) if <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3cd878e0-18a2-4b5f-ab82-09f76d8a3ceb.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\01cce854-1826-4603-bf1a-335625a00779.png" xlink:type="simple"/></inline-formula>.</p><p>The norm of a vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\54f00e27-af0f-4350-ac79-1d571d79370d.png" xlink:type="simple"/></inline-formula> is defined by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\000cfb26-122f-4adf-aafd-492072dde982.png" xlink:type="simple"/></inline-formula>. Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\ebef1f9b-bb06-45bb-9446-ba4487e5f2e2.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4f0103cf-2482-4463-8a3b-30a9e1e23c40.png" xlink:type="simple"/></inline-formula> be two vec-</p><p>tors in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\2b4b47e5-88b3-4fe9-bb74-2b7ec3d568d9.png" xlink:type="simple"/></inline-formula>, then the Lorentzian cross product of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9c3dda44-b65c-49e3-a3c7-3bccd1ac9aef.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\119299b8-f83b-4c88-8c45-63cb765a8013.png" xlink:type="simple"/></inline-formula> is given by</p><disp-formula id="scirp.47947-formula3349"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e5e56e27-2ec9-4bff-8d98-22131adc46e3.png"/></disp-formula><p>If <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\91c2f8fd-a207-4a6a-833b-39f4efcb02cf.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\190bbb38-5bfe-4f50-badf-890d0be5d4cb.png" xlink:type="simple"/></inline-formula> are real numbers and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d40b013a-94a4-4de0-b9d3-aa37d5a30dc8.png" xlink:type="simple"/></inline-formula>, the combination <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8c2ead7d-db4f-47f9-b33c-e099ca74e3d9.png" xlink:type="simple"/></inline-formula> is called a dual number, where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7627085f-29e6-4687-ad01-fafe6e9b9e00.png" xlink:type="simple"/></inline-formula> is a dual unit.</p><p>The set of all dual numbers forms a commutative ring over the real numbers field and is denoted by 𝔻. Then the set</p><disp-formula id="scirp.47947-formula3350"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d8fa27f5-4344-458e-8338-be1e5e17e148.png"/></disp-formula><p>is a module over the ring 𝔻 which is called a 𝔻-module or dual space. The elements of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\afd53375-0519-4dff-94a1-8a0d4fd94cac.png" xlink:type="simple"/></inline-formula> are called dual vectors. Thus a dual vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\50038360-60cd-4123-bc07-f42e0d903f88.png" xlink:type="simple"/></inline-formula> can be written as</p><disp-formula id="scirp.47947-formula3351"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0a87b014-237f-4010-8141-26137c4657ff.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f389ca73-28da-4af9-900d-719d6ce5c52c.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0ed7ba47-17da-4c9e-9ef9-45d83bd7f188.png" xlink:type="simple"/></inline-formula> are real vectors at<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7238d6f4-90d7-4fe5-8f87-adbf8a8bd0d5.png" xlink:type="simple"/></inline-formula>.</p><p>If <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\23c4f4e9-7056-49a6-a835-f1d32cf380fa.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\46629ff4-95be-417c-ab42-cc33579c0b94.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9146ee50-9985-4616-947f-f50a3ca13ff0.png" xlink:type="simple"/></inline-formula> then the division is given by</p><disp-formula id="scirp.47947-formula3352"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\be843b59-4c04-4ce7-9aac-92ad898e7eea.png"/></disp-formula><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\94df0612-3de0-4e15-a376-bed88944a0a8.png" xlink:type="simple"/></inline-formula> be a differentiable function with dual variable<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\614fa557-7954-4567-9a47-928422d75dbb.png" xlink:type="simple"/></inline-formula>. Then the Maclaurin series generated by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\479dea51-c16d-45fe-a9bb-4c869e828640.png" xlink:type="simple"/></inline-formula> is</p><disp-formula id="scirp.47947-formula3353"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e160e9f5-3eb8-46ad-9ebd-a96caba156c6.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8c5419c9-9f36-4bc4-9f42-1f17a6774773.png" xlink:type="simple"/></inline-formula> is the derivative of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6a13baa1-f578-46d9-839a-edfa36def46d.png" xlink:type="simple"/></inline-formula>. Then it is easy to see that</p><disp-formula id="scirp.47947-formula3354"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\da49f304-0edc-4641-833c-fa9c14cca164.png"/></disp-formula><disp-formula id="scirp.47947-formula3355"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\da49f304-0edc-4641-833c-fa9c14cca164.png"/></disp-formula><disp-formula id="scirp.47947-formula3356"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\da49f304-0edc-4641-833c-fa9c14cca164.png"/></disp-formula><p>The norm <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\1a01978d-3d28-4950-860f-7483577e1437.png" xlink:type="simple"/></inline-formula> of a dual number <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\fdde2a83-6222-4e48-9fc9-01114573aea6.png" xlink:type="simple"/></inline-formula> is defined by</p><disp-formula id="scirp.47947-formula3357"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9c1c850e-18da-417c-9a5c-f6b2898ca891.png"/></disp-formula><p>Then we can write</p><disp-formula id="scirp.47947-formula3358"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\29c09947-55dc-43c3-89fd-a7ba482a0116.png"/></disp-formula><p>The Lorentzian inner product of two dual vectors<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\92eeac23-a0df-4f8b-b47d-c9b66d38d925.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\fa13b141-96c1-4e46-a624-fb298b99badd.png" xlink:type="simple"/></inline-formula>is defined by</p><disp-formula id="scirp.47947-formula3359"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7def24b8-935c-4525-98cf-449b8e17a2dc.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\70c6cadc-d64d-4621-ae1d-c9bb0607cd57.png" xlink:type="simple"/></inline-formula> is the Lorentzian inner product of the vectors <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4e7b48b6-73a0-4538-8ad9-652929f70454.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3d805dc1-cf9b-44a1-9364-94942092e6e3.png" xlink:type="simple"/></inline-formula> in the Minkowski 3-space<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b19be182-e7df-4f60-ae99-70cd74d18967.png" xlink:type="simple"/></inline-formula>.</p><p>A dual vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\5761a042-fa75-4f63-8797-1fbe235cf7a4.png" xlink:type="simple"/></inline-formula> is said to be timelike if<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d410c0e7-7af4-4961-ade4-46409c059a03.png" xlink:type="simple"/></inline-formula>, spacelike if <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\2e1f0af0-553f-4910-82d9-4faff87712cc.png" xlink:type="simple"/></inline-formula> and lightlike (or null) if</p><disp-formula id="scirp.47947-formula3360"><label>,</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\84f1c69d-9a50-4385-b646-ce674e3a98dc.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\adbdb8b7-2699-471f-9be7-dc72211556ca.png" xlink:type="simple"/></inline-formula> is a Lorentzian inner product with signature<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4676c667-a597-4467-abe1-9f7ebf78cf4e.png" xlink:type="simple"/></inline-formula>.</p><p>The set of all dual Lorentzian vectors is called dual Lorentzian space and it is denoted by</p><disp-formula id="scirp.47947-formula3361"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7646e420-22cb-4762-9211-e7ac6bf68359.png"/></disp-formula><p>The Lorentzian cross product of dual vectors <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\204775ef-cd0b-411c-a930-3c6715d1d2e5.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d1be9c4e-5d18-4e8a-b6d3-f2a9878e56d4.png" xlink:type="simple"/></inline-formula> is defined by</p><p>Lemma 2.1. Let<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e7a69891-1eba-4d47-ae7a-7deb51dfb341.png" xlink:type="simple"/></inline-formula>. Then [<xref ref-type="bibr" rid="scirp.47947-ref12">12</xref>]</p><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6c593700-8db3-4e61-b2a0-2b812e227b4c.png" xlink:type="simple"/></inline-formula> is the Lorentzian cross product in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3475a5db-c5fc-4a24-97f9-056069dafa24.png" xlink:type="simple"/></inline-formula>.</p><p>Lemma 2.1. Let<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e7a69891-1eba-4d47-ae7a-7deb51dfb341.png" xlink:type="simple"/></inline-formula>. Then [<xref ref-type="bibr" rid="scirp.47947-ref12">12</xref>]</p><p>1) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\05d37b59-8019-406e-a0f1-b7b41881c4ad.png" xlink:type="simple"/></inline-formula></p><p>2) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\03ec16db-0ea8-4dd6-a03a-1447c2ca01b3.png" xlink:type="simple"/></inline-formula>; and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\99e61464-9f8c-4114-9be6-06a48cc76698.png" xlink:type="simple"/></inline-formula>,</p><p>3) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\347884a9-7317-4276-ac6e-2cf7fab63b68.png" xlink:type="simple"/></inline-formula>,</p><p>4) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\26b312f0-445d-40a0-ac05-abf691878da5.png" xlink:type="simple"/></inline-formula>.</p><p>Let<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\53642031-f4ff-41be-b724-419f74940ba9.png" xlink:type="simple"/></inline-formula>. Then <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\72fe4072-ed66-4a10-a6c5-8e30a9306249.png" xlink:type="simple"/></inline-formula> is said to be dual timelike unit vector (resp., dual spacelike unit vector) if the vectors <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\090b13fb-e9b4-4211-a402-9f01b1d5d5f9.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\1a9f1696-df3b-4f8c-bc6a-649d270c7c83.png" xlink:type="simple"/></inline-formula> satisfy the following properties:</p><p><img src="htmlimages\12-1720166x\c742c362-0e7e-4a31-81cf-3b2f6ebbc752.png" width="115" height="42.5" />, (resp.,<img src="htmlimages\12-1720166x\e8ffcc23-1419-4cd8-b472-036454550570.png" width="96.25" height="42.5" />), <img src="htmlimages\12-1720166x\a94f66dd-da9f-47a6-9fac-a7a77065884c.png" width="117.5" height="47.5" /></p><p>The set of all dual timelike unit vectors (resp., all dual spacelike unit vectors) is called the dual hyperbolic unit sphere (resp., dual Lorentzian unit sphere) and is denoted by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\408c5538-a498-4f9c-819e-9c8af73549dd.png" xlink:type="simple"/></inline-formula> (resp.,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7dd73376-cdd1-4449-8368-939efced43ce.png" xlink:type="simple"/></inline-formula>) [<xref ref-type="bibr" rid="scirp.47947-ref6">6</xref>] . (See [<xref ref-type="bibr" rid="scirp.47947-ref13">13</xref>] -[<xref ref-type="bibr" rid="scirp.47947-ref16">16</xref>] for Lorentzian basic concepts.)</p><p>Theorem 2.2. (E. Study Map) [<xref ref-type="bibr" rid="scirp.47947-ref6">6</xref>] There exists one-to-one correspondence between directed timelike (resp., spacelike) lines of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\476cfe49-85e0-41e4-bff7-070ec5831fd7.png" xlink:type="simple"/></inline-formula> and an ordered pair of vectors <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f6b6aed6-4c35-4be8-9ace-b6195cfa64ee.png" xlink:type="simple"/></inline-formula> such that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3e9fbe12-4e8f-4b67-89a3-6a5ebaa4b316.png" xlink:type="simple"/></inline-formula> (resp.,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\10dbbfb5-6d5d-496d-8222-54e021a768dd.png" xlink:type="simple"/></inline-formula>) and</p><disp-formula id="scirp.47947-formula3362"><label>.</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\18e6339c-0964-4c0c-9dc1-09c8bddbf7b2.png"/></disp-formula><p>Definition 2.1. A directed timelike line in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4320192e-9f02-415c-b224-e179ad14bb13.png" xlink:type="simple"/></inline-formula> may be given by two points on it, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\49e9c4c2-836f-4d90-8c2b-ac45386058b5.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\37095350-e323-4e63-86a6-d53cd6f8ce2c.png" xlink:type="simple"/></inline-formula>. If <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\fdc2f29b-9aa6-43dd-9115-ec0ad296380e.png" xlink:type="simple"/></inline-formula> is any non-zero constant, the parametric equation of the line is<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d6554e14-476d-4a07-a5bd-5527828b4e98.png" xlink:type="simple"/></inline-formula>. In this case, the vector given by</p><disp-formula id="scirp.47947-formula3363"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\5b7327f7-5104-4426-8645-476fe4f8fbc7.png"/></disp-formula><p>is called the moment of the vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\2be389db-47ca-44fe-b6b0-e7711387fb7c.png" xlink:type="simple"/></inline-formula> with respect to the origin 0.</p><p>This means that the direction vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0812dc25-ba42-4677-b6c2-3414654ee800.png" xlink:type="simple"/></inline-formula> of the timelike line and its moment vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\11178243-fdbe-4bbc-bc08-5a4b28a19b9e.png" xlink:type="simple"/></inline-formula> are independent of the choice of the points <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8e88c36b-58d9-445c-958a-63e7efe59069.png" xlink:type="simple"/></inline-formula> on the line. However the vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\1c90e437-d6b2-47b5-95a8-a3cd83e527f3.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3c35e29b-0fe4-4073-83c0-2c28a532c33a.png" xlink:type="simple"/></inline-formula> are not independent of one another. Also, they satisfy the following properties:</p><disp-formula id="scirp.47947-formula3364"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\5e782b27-1b65-460c-874e-624968d86095.png"/></disp-formula><p>Let<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8fd63045-5319-4d4f-8328-62f581c7f288.png" xlink:type="simple"/></inline-formula>, 0 and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\725899eb-cb9e-4029-a6d0-93095a18256c.png" xlink:type="simple"/></inline-formula> denote the dual hyperbolic unit sphere, the center of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\51792c91-f6c1-4fd8-a2f1-45f1e92a6b87.png" xlink:type="simple"/></inline-formula> and the dual orthonormal system at 0, respectively where we have</p><disp-formula id="scirp.47947-formula3365"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0071a024-ce18-46bf-93c6-30ea09b24289.png"/></disp-formula><disp-formula id="scirp.47947-formula3366"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0071a024-ce18-46bf-93c6-30ea09b24289.png"/></disp-formula><p>and</p><disp-formula id="scirp.47947-formula3367"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c20a056f-7c62-4998-aeb7-75d8e0417e2c.png"/></disp-formula><p>[<xref ref-type="bibr" rid="scirp.47947-ref7">7</xref>] . In this case the orthonormal system <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\757edc78-1ff6-4e3d-af2e-a38709573c75.png" xlink:type="simple"/></inline-formula> is the system of the space of lines<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8b50e7e0-205a-4aec-ae5c-2659867c3286.png" xlink:type="simple"/></inline-formula>.</p><p>A ruled surface is a surface generated by the motion of a straight line in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\2f09c3cd-1d2d-4530-9e18-f72bffb599e2.png" xlink:type="simple"/></inline-formula>. This line the generator of the surface. This follows the following definition.</p><p>Definition 2.2. A ruled surface is said to be timelike if the normal of surface at every point is spacelike, and spacelike if the normal of surface at every point is timelike [<xref ref-type="bibr" rid="scirp.47947-ref7">7</xref>] .</p><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\1e049ddf-2c97-4b1b-8f52-1c6523f92ab5.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3ddda81c-1d3e-4f9e-880d-d93ce3f2c845.png" xlink:type="simple"/></inline-formula> denote two different points at <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6e2a3970-6ac5-4419-a6df-7e4e9286abc6.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0adf38a2-58b5-47a1-9c78-45f3ec0535c7.png" xlink:type="simple"/></inline-formula> denote the dual hyperbolic angle<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d113d609-c6f8-4ee4-9647-5db25970bca1.png" xlink:type="simple"/></inline-formula>. The hyperbolic angle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e112d1a4-9c5f-4158-9ff9-b2681aa1ff88.png" xlink:type="simple"/></inline-formula> has a value <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\321f2bab-7224-40e6-a446-cd857a05425f.png" xlink:type="simple"/></inline-formula> which is a dual number, where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\82758a58-22e9-479c-9829-cab70dd3918c.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8c10e3a5-a829-42b9-a825-652f336654da.png" xlink:type="simple"/></inline-formula> are the hyperbolic angle and the minimal Lorentzian distance between directed lines <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\808f26a5-c6f6-4d97-ba42-5158405f6827.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0fa06800-2a03-490a-9637-7ff07ddb0fe2.png" xlink:type="simple"/></inline-formula>, respectively.</p></sec><sec id="s3"><title>3. Dual Curvature Motion on the Dual Hyperbolic Unit Sphere <img src="htmlimages\12-1720166x\384ce438-6de2-4ac7-9be8-56a92a1aaf4d.png" width="47.5" height="51.25" /></title><p>Let us consider a fixed dual orthonormal frame <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\a64f7112-6296-4eae-a5e1-1f83c25a4c60.png" xlink:type="simple"/></inline-formula> and represent this frame by the dual hyperbolic unit sphere<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3e3c63bb-f902-41c4-8830-b374407e72a5.png" xlink:type="simple"/></inline-formula>. Consider the dual hyperbolic spherical motion of a hyperbolic spherical segment</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0162bc78-a511-4663-851c-37cbad8bd44c.png" xlink:type="simple"/></inline-formula>of constant such that its endpoints move along circles, one of them being a great circle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\2761481b-77cc-4593-95e3-3d8fb15d9c0b.png" xlink:type="simple"/></inline-formula> which lying on the plane <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\db47c1b7-fa9d-44b8-b7de-26b1c8bb5de0.png" xlink:type="simple"/></inline-formula> on<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f3a4854d-80e0-4b57-aa3a-47e6c4b30055.png" xlink:type="simple"/></inline-formula>. Let a circle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\dbf0d774-0e97-4f57-9416-944eb9694096.png" xlink:type="simple"/></inline-formula> with radius <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b99e4940-83c2-4846-be4a-31cd600067db.png" xlink:type="simple"/></inline-formula> which is perpendicular to the great circle</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6444710a-0d33-45c6-8228-9df0727e75c4.png" xlink:type="simple"/></inline-formula>be given in a plane which is parallel to the plane<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\eae24040-f8ea-4ee4-ba1e-61b858d0be41.png" xlink:type="simple"/></inline-formula>. Its center is on the vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\ef82eda0-54c8-4dc5-98ae-a8fafb614f21.png" xlink:type="simple"/></inline-formula> and with distance</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\ca157212-f121-4f0f-bf5a-a7137636a91d.png" xlink:type="simple"/></inline-formula>from the plane<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4ecd2bc3-952b-44f3-9053-8235dd1499b4.png" xlink:type="simple"/></inline-formula>. The segment <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\fe69c066-bc13-44ac-a947-572a6e4e6a97.png" xlink:type="simple"/></inline-formula> moves so that<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\bc3a1dc2-ae02-42f8-9828-9fcc67fb9013.png" xlink:type="simple"/></inline-formula>. The position vectors of the</p><p>endpoints of segment <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c3f223f9-6c87-4a7e-a650-20e6c3a6f4d6.png" xlink:type="simple"/></inline-formula> are chosen as the vectors <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3a635926-e6e8-4023-aeb6-47325e44c6ff.png" xlink:type="simple"/></inline-formula> (timelike) and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b373cdd2-e430-4b5a-a65a-b3567594fa77.png" xlink:type="simple"/></inline-formula> (spacelike) of the moving frame<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\1235b807-49a0-40b3-b3a0-948344d36e5c.png" xlink:type="simple"/></inline-formula>. The vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7347035d-a9df-4e77-ad7f-25156c6bb74d.png" xlink:type="simple"/></inline-formula> is then defined by the relation<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0d5baf5e-cda5-47be-b37a-842d48808fc2.png" xlink:type="simple"/></inline-formula>. As the parameter of motion we choose the dual hyperbolic angle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9df55ccc-d168-40d1-8aa2-2e0d485c257a.png" xlink:type="simple"/></inline-formula> of the timelike vectors <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\92fbf3bd-4aa0-4d01-95b2-59e8719de068.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8414d0d2-313e-4841-a440-c4c78169a129.png" xlink:type="simple"/></inline-formula>. Let us denote the dual hyperbolic angle of the vectors <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6e2b28fe-7dab-42c2-b526-ecfda8125211.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f83129b7-2d52-457d-8583-2ef19d240299.png" xlink:type="simple"/></inline-formula> by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\74fdf74c-e597-4eff-a20d-7ef395a9030b.png" xlink:type="simple"/></inline-formula>. Then</p><disp-formula id="scirp.47947-formula3368"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\671c2574-bd77-4f43-b3ac-2b2f9edfb28f.png"/></disp-formula><p>where the vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\db455abe-eba9-4add-8a3b-51f240337745.png" xlink:type="simple"/></inline-formula> is spacelike. Further, we have</p><p><img src="htmlimages\12-1720166x\f222f43d-6530-4b70-a7b9-093b07edcf72.png" width="192.5" height="37.5" />(<img src="htmlimages\12-1720166x\54ee1a71-170c-4320-b67c-97323f59f967.png" width="30" height="37.5" />timelike).</p><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\861fb329-23c9-465d-a314-c4b25c3059cf.png" xlink:type="simple"/></inline-formula> is timelike. It must be</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\327d6ec1-d34f-4bd4-941f-e7ca59b13e50.png" xlink:type="simple"/></inline-formula>, i.e., <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\2797b523-0d51-4fa4-9d54-79726c7b46f0.png" xlink:type="simple"/></inline-formula></p><p>i.e. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\95eb1898-d1c2-4422-bbee-6e9ebec8b748.png" xlink:type="simple"/></inline-formula>or<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e7bbe634-df0d-46eb-a96a-f3419abd1579.png" xlink:type="simple"/></inline-formula>, where<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\71007df4-aa4c-4089-ac89-d9c7deb259fb.png" xlink:type="simple"/></inline-formula>. Then<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e18bae20-5800-4d01-84dd-827b5e0cf5c5.png" xlink:type="simple"/></inline-formula>. Thus we obtain</p><disp-formula id="scirp.47947-formula3369"><label>(1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f9b28195-be44-4b1b-8191-d77a9fb0812e.png"/></disp-formula><p>Thus, we have the orthonormal dual frame<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\db567536-16d1-48af-856e-1413caede956.png" xlink:type="simple"/></inline-formula>. Let this system be represented by moving hyperbolic sphere<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c89d67d8-d1cb-4a68-91ea-0f442c844f0f.png" xlink:type="simple"/></inline-formula>. Then, a dual hyperbolic curvature motion <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\5422b525-e2f3-4599-b728-5c362575e04f.png" xlink:type="simple"/></inline-formula> takes place. This motion will be called a dual hyperbolic curvature motion. Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\885e4bf0-792b-4619-bec8-b1601dd5633f.png" xlink:type="simple"/></inline-formula> be a fixed point on the arc<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\881d832b-d4cd-43b5-94f3-88defb23f9e2.png" xlink:type="simple"/></inline-formula>. During the dual hyperbolic curvature motion, the point <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7f8a2565-f275-4ac3-89da-2ccbc1076734.png" xlink:type="simple"/></inline-formula> draws an orbit on the fixed hyperbolic sphere<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\06fad2b4-188f-4951-81bc-dac088df2b83.png" xlink:type="simple"/></inline-formula>.</p><p>Denote the dual hyperbolic angles of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c0e55d91-1841-49d0-b2cf-ead6c1a42402.png" xlink:type="simple"/></inline-formula> by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\31adb443-be67-48c1-80f1-dca7cba892fd.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\738b0ed6-d5ba-4696-ab52-8e4e343f3c81.png" xlink:type="simple"/></inline-formula> respectively. Then it can be written</p><disp-formula id="scirp.47947-formula3370"><label>(2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\00a2a216-0cdb-4b14-94bd-02a80ea4298c.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6a74e46c-d719-4e5b-b1eb-b629b5e388df.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.47947-ref5">5</xref>] . From Equation (2), making the necessary calculations for<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b6cf5bbd-5f14-4b43-9e53-81dc831fc8cd.png" xlink:type="simple"/></inline-formula>, we have</p><disp-formula id="scirp.47947-formula3371"><label>(3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b8c9c99f-612d-4a34-a24a-fbe00b377093.png"/></disp-formula><disp-formula id="scirp.47947-formula3372"><label>(4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\86525833-8fcb-4e28-a8d2-191fa235da58.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\85d9a813-17a7-4dc1-998e-780bb3f0c696.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8e3922e3-3d4e-4c7f-8d4c-81ccc483dce4.png" xlink:type="simple"/></inline-formula> are the real and dual parts of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8a9d046f-cbf3-445f-9118-020d7bbae0e1.png" xlink:type="simple"/></inline-formula>, also. Since, Ө<sub>1</sub> and Ө<sub>2</sub> are constant (i.e.<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c3cc616f-db13-4eea-b5df-d524074145c7.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6ee83659-8d9e-4ef8-b10b-4ff6e5867559.png" xlink:type="simple"/></inline-formula>are all constants), <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b5820e5a-84a6-4ca7-bdb8-e0d2521f8787.png" xlink:type="simple"/></inline-formula>is constant. Equations (3) and (4) depend only two parameters <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b57cf4a2-2608-4631-839c-c0ecb16b1499.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\ea8cbbf8-8355-48bc-a66c-d0baa2d35b47.png" xlink:type="simple"/></inline-formula>. Thus, Equations (3) and (4) represent a timelike congruence in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c744f18c-7468-47f2-97e0-1ff1a54016c1.png" xlink:type="simple"/></inline-formula> (for more details on congruences, see [<xref ref-type="bibr" rid="scirp.47947-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.47947-ref12">12</xref>] ).</p><p>Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\adf45452-fde5-4425-a228-d0ca2ea802c9.png" xlink:type="simple"/></inline-formula> denote the position vector of an arbitrary point <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9f51ae99-d082-48a0-bbac-ed629ccf1225.png" xlink:type="simple"/></inline-formula> of a directed timelike line of this timelike line congruence in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\113865c9-44d4-4ae9-82ac-e9037fd7c25e.png" xlink:type="simple"/></inline-formula>. Then we have</p><disp-formula id="scirp.47947-formula3373"><label>(5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9d5959a8-a15e-42f6-884f-5e30ebee7de5.png"/></disp-formula><p>Since <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\cf4a0dbe-1229-4336-b381-63bdb931e409.png" xlink:type="simple"/></inline-formula> are the coordinates of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\17186930-fe1d-4f2a-83c5-dca23b3cce2b.png" xlink:type="simple"/></inline-formula>, making the necessary calculations, we obtain</p><disp-formula id="scirp.47947-formula3374"><label>(6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\070d709a-5858-469c-8701-0e1058a0a1f8.png"/></disp-formula><disp-formula id="scirp.47947-formula3375"><label>(7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\37cabed9-0a0f-4a59-b471-678b081613fc.png"/></disp-formula><p>and</p><disp-formula id="scirp.47947-formula3376"><label>(8)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f3f57724-027d-418b-a004-0cebfa644f33.png"/></disp-formula><p>If<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\ca210940-bb46-47e9-85b9-54e5650758df.png" xlink:type="simple"/></inline-formula>, (i.e.<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\dd54ac9a-5d63-48e9-9caa-88a4959d5703.png" xlink:type="simple"/></inline-formula>) then<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\af9b798a-3a8b-4b9f-81dc-7315e24fddb7.png" xlink:type="simple"/></inline-formula>, i.e.<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\95d37655-e13f-4e9d-a19d-6fbc63b89610.png" xlink:type="simple"/></inline-formula>. In this case, from Equation (2) we have<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\a697a022-5430-4d58-b198-60036b2253db.png" xlink:type="simple"/></inline-formula>. Thus, from Equations (6)-(8) we obtain</p><disp-formula id="scirp.47947-formula3377"><label>(9)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d6e3d398-58ac-44bc-a284-9788f3cdd24e.png"/></disp-formula><p>From Equation (9) we have</p><disp-formula id="scirp.47947-formula3378"><label>(10)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\5e7ed511-7d76-44df-8380-593a8743d7b7.png"/></disp-formula><p>which represents a line congruence. Thus, we have the following theorem.</p><p>Theorem 3.1. During the dual hyperbolic spherical curvature motion <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\2653495b-a3f3-40b5-a1ba-ff57a33af24d.png" xlink:type="simple"/></inline-formula> in the case of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\456ed5a0-605b-4092-b8fc-b9d17bbbbb68.png" xlink:type="simple"/></inline-formula> (hence<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\16f0e3c0-7c89-4aaa-93f4-aff55921cbf9.png" xlink:type="simple"/></inline-formula>) in Equation (2), the Study map of the orbit which is drawn on the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\785276a5-ea84-4af3-b7c9-2ddfdb322b6c.png" xlink:type="simple"/></inline-formula> by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\27975f1a-fab2-43e1-9940-26bcd4e211b2.png" xlink:type="simple"/></inline-formula> is the congruence in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\eba894aa-ec52-4bc4-850a-9c08d347dc98.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.47947-formula3379"><label>(11)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4c366ed9-5634-4bdd-ab91-ec31566ef165.png"/></disp-formula><p>If we take <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9677dfec-76c8-4c81-ac19-ad29d9a5f5a4.png" xlink:type="simple"/></inline-formula> in the Equation (9), then we have</p><disp-formula id="scirp.47947-formula3380"><label>(12)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\cb14b96b-9904-4685-87d6-5ba17e96dd3b.png"/></disp-formula><p>Thus, we have the following theorem.</p><p>Theorem 3.2. During the dual hyperbolic spherical curvature motion <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\cd8b64ea-9f62-413f-98d2-6240642abece.png" xlink:type="simple"/></inline-formula> in the case of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\6329c3b2-dc51-4353-952a-8c4061e4dc8b.png" xlink:type="simple"/></inline-formula>, the Study map in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f244d090-4823-4d0b-ae9a-fc64568793eb.png" xlink:type="simple"/></inline-formula> of the orbit drawn on the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\bbed26fe-ce6d-4364-9ff0-61c922b60acb.png" xlink:type="simple"/></inline-formula> by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9791be5c-d674-4903-bf91-63aa963c9956.png" xlink:type="simple"/></inline-formula> is the cone which is given by</p><disp-formula id="scirp.47947-formula3381"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c68d2b5b-da81-4a51-b5d5-a37c9d9ef143.png"/></disp-formula><p>In addition, if we take <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\345980b8-370f-4c6b-baf9-834397bf292e.png" xlink:type="simple"/></inline-formula> (c = constant) then we have</p><disp-formula id="scirp.47947-formula3382"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3e07dd9c-6f7d-4b43-b4eb-74f75a2f6b55.png"/></disp-formula><p>which represents a right helicoid.</p><p>If<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\55440724-c130-4c62-9855-bf2e0d197118.png" xlink:type="simple"/></inline-formula>, i.e.<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f797419d-04a4-488e-af6d-1f3ee47d40f6.png" xlink:type="simple"/></inline-formula>, then<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e8f1cba3-db36-4f50-baa5-e76272b073f5.png" xlink:type="simple"/></inline-formula>, i.e. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\cdb257b5-1021-4d7b-811b-b105ef7489b0.png" xlink:type="simple"/></inline-formula>In this case , from Equation (2) we have<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\57feac0f-1c45-4022-abd2-92f0fb8fd95f.png" xlink:type="simple"/></inline-formula>. Thus, from Equations (6)-(8) we obtain</p><disp-formula id="scirp.47947-formula3383"><label>(13)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\be936d2f-a4f8-4da1-9c6a-030bb2612152.png"/></disp-formula><p>If we put<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9cd7ea95-f438-4688-ae05-f5ff25b4ce40.png" xlink:type="simple"/></inline-formula>, from Equation (13) we have</p><disp-formula id="scirp.47947-formula3384"><label>(14)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\885ee7ca-2be3-401d-89d0-ff16c9d792a2.png"/></disp-formula><p>From Equation (14) we have</p><disp-formula id="scirp.47947-formula3385"><label>(15)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\2498dfe3-c614-4a92-aab3-fb3297ce3fa1.png"/></disp-formula><p>which represents a cone whose axis is the vector<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\a5aa635d-3d3b-44e2-bd2e-df62bb9c7aa2.png" xlink:type="simple"/></inline-formula>. Thus, we have the following theorem.</p><p>Theorem 3.3. During the dual hyperbolic spherical curvature motion, the orbit drawn on <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0b7ad4c0-62e9-4985-add8-0f1143ee3fc8.png" xlink:type="simple"/></inline-formula> by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\574f7487-3486-4cbd-b82d-9a8ea19fdc45.png" xlink:type="simple"/></inline-formula> (if<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0c4d5dfc-bc7c-4f69-bb7b-6919c999cc8c.png" xlink:type="simple"/></inline-formula>) represents a cone in the<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c4e6b7cb-1d03-4f9b-a3a9-d66023967858.png" xlink:type="simple"/></inline-formula>, whose axis is the vector<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\8b5dabf3-d629-4c83-bc6c-78650cb07699.png" xlink:type="simple"/></inline-formula>.</p><p>If we put<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\cd18624f-2e95-4a28-afac-93e2fbc75a0e.png" xlink:type="simple"/></inline-formula>, from Equation (13) we have</p><disp-formula id="scirp.47947-formula3386"><label>(16)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c1d2328a-25de-4a94-baea-eda9459c0e0f.png"/></disp-formula><p>From Equation (16) we have</p><disp-formula id="scirp.47947-formula3387"><label>(17)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\85618fbf-6d44-49cb-a04b-45362d161c26.png"/></disp-formula><p>which represents a cone whose axis is the vector<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\08ef3ef8-da57-4c79-8f57-f0ad32bd3014.png" xlink:type="simple"/></inline-formula>. Thus, we have the following theorem.</p><p>Theorem 3.4. During the dual hyperbolic spherical curvature motion, the orbit drawn on <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\94f6bb24-3c23-4787-a752-e060b4b74e37.png" xlink:type="simple"/></inline-formula> by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\5fc088f0-4c16-46ab-8ade-34d90c3b5ae9.png" xlink:type="simple"/></inline-formula> (if<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e63e8656-a3e8-4ed6-ba48-f0fc5c6bd949.png" xlink:type="simple"/></inline-formula>) represents a cone in the<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\051640a1-872b-40de-822c-d9b4cec66803.png" xlink:type="simple"/></inline-formula>, whose axis is the vector<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\e9ebe1d1-6084-41de-805d-e1050aabcd4e.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s4"><title>4. Analysis of the Orbit of <img src="htmlimages\12-1720166x\30d885dc-13ad-4c10-8bb1-39c699623d54.png" width="32.5" height="47.5" /> during the Dual Hyperbolic Spherical Curvature Motion</title><p>Seperating real and dual parts of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c37d7114-324a-4519-acb9-09c28b807fc8.png" xlink:type="simple"/></inline-formula>, from Equation (1) we have</p><disp-formula id="scirp.47947-formula3388"><label>(18)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3050838f-da51-47df-b713-537965a460c4.png"/></disp-formula><disp-formula id="scirp.47947-formula3389"><label>(19)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f70b7106-6eda-4814-8f77-1a861011bf03.png"/></disp-formula><p>Equations (18) and (19) have only two parameters <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\aeb7d637-9299-44da-8e6f-2f5c2c667c1c.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\12907b65-8fd3-438d-82cd-1c0f441ea6c0.png" xlink:type="simple"/></inline-formula>. Hence Equations (18) and (19) represent a line congruence in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\7a877ee7-bea7-4535-a068-868f6f26c079.png" xlink:type="simple"/></inline-formula>. Let <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\9b96c04e-d966-4d59-b34d-e08a0b03a480.png" xlink:type="simple"/></inline-formula> denote the position vector of an arbitrary point <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\3d7a8c39-39af-4c8e-b05d-c514b3a34827.png" xlink:type="simple"/></inline-formula> of an oriented line of this congruence in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\36d339e9-cf9a-4ebb-9fa0-0e786fcb5270.png" xlink:type="simple"/></inline-formula>, then considering Equation (5) we have</p><disp-formula id="scirp.47947-formula3390"><label>(20)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\0f78d7c3-ec8f-4b3d-bcbd-5f320d0d3dd8.png"/></disp-formula><p>Since <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\64ed99e5-8bb9-4d37-9d2e-3771dca2f56d.png" xlink:type="simple"/></inline-formula> are the coordinates of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\326bf603-b848-4525-9cb8-246134ecc993.png" xlink:type="simple"/></inline-formula>, making the necessary calculations, we obtain</p><disp-formula id="scirp.47947-formula3391"><label>(21)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\49ff417f-d511-4305-8a5d-4ffbf4b244b2.png"/></disp-formula><p>In the case of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\56d0f848-b072-4541-a389-405d90a4477e.png" xlink:type="simple"/></inline-formula> from Equation (21) we have</p><disp-formula id="scirp.47947-formula3392"><label>(22)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\c23ca68a-03a0-4fb1-8590-0db4d0a32be9.png"/></disp-formula><p>From Equation (22) we obtain</p><disp-formula id="scirp.47947-formula3393"><label>(23)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f62ef4f7-b95e-4e7e-8905-cd57f3ced621.png"/></disp-formula><p>which represents an one-parameter family of cone in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\39dcee88-c3ae-434c-92ae-b4263af3be50.png" xlink:type="simple"/></inline-formula>.</p><p>If we put <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\10cca379-d7d1-4cdb-a82a-7c9668b64482.png" xlink:type="simple"/></inline-formula> in the Equation (23), then we have</p><disp-formula id="scirp.47947-formula3394"><label>(24)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\88a94c32-dc04-4c02-9369-a39a16d0a22a.png"/></disp-formula><p>which represents an elliptic cone, whose axis is the vector<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\967fcb4e-c076-4a3f-8734-1b81a10c0d22.png" xlink:type="simple"/></inline-formula>. Thus, we have the following theorem.</p><p>Theorem 4.1. During the dual hyperbolic spherical curvature motion, the orbit drawn on <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\88fa5ce6-4e55-4335-80a9-384db127563d.png" xlink:type="simple"/></inline-formula> by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\5099cd8d-278e-4276-974f-ed7cfd83b75b.png" xlink:type="simple"/></inline-formula> (if<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b9a818e6-d590-4413-9526-545a3eef2bd5.png" xlink:type="simple"/></inline-formula>) represents an elliptic cone, whose axis is the vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\65fbff31-cf6a-425a-a34e-5efe81b9817e.png" xlink:type="simple"/></inline-formula> in the<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\b2d50818-5f97-4b63-99dc-51debbd9cee6.png" xlink:type="simple"/></inline-formula>.</p><p>In addition, putting various values of parameters in the Equations (21) or (22) we have different line congruences or ruled surfaces in<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\f8f5954c-583b-4548-962b-c98eb601c0da.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s5"><title>5. Conclusion</title><p>This paper presents the curvature motion on the dual hyperbolic unit sphere<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d8646dd2-1149-44d7-804d-106ae8db23c9.png" xlink:type="simple"/></inline-formula>. We define the curvature motion on the dual hyperbolic unit sphere <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\ccee676e-f5d2-4eb1-bb28-c7ec36440324.png" xlink:type="simple"/></inline-formula> of the dual Lorentzian space <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\155415de-8ec6-41eb-a234-5104651309a6.png" xlink:type="simple"/></inline-formula> and the results are carried over to the Lorentzian line space by the E. Study mapping. The orbits drawn on the fixed dual hyperbolic unit sphere by unit dual vectors of an orthonormal base <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\d8850721-b93d-47e2-94e9-8d90f2ea265d.png" xlink:type="simple"/></inline-formula> are obtained. During this carrying, we do an analysis of orbits they drawn by the vectors <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\12-1720166x\4c359bca-1a9c-4b0e-919a-245663113076.png" xlink:type="simple"/></inline-formula> of dual hyperbolic unit sphere and then we get some line congruences, the families of ruled surfaces and ruled surfaces in according to variables of parameters. Moreover we find equations of these line congruences, the families of ruled surfaces and ruled surfaces. 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