<?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">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2016.716204</article-id><article-id pub-id-type="publisher-id">JMP-72940</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>
 
 
  New Expansion Dynamics Applied to the Planar Structures of Satellite Galaxies and Space Structuration
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Jacques</surname><given-names>Fleuret</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Independent Researcher, Antony, France</addr-line></aff><author-notes><corresp id="cor1">* E-mail:</corresp></author-notes><pub-date pub-type="epub"><day>05</day><month>12</month><year>2016</year></pub-date><volume>07</volume><issue>16</issue><fpage>2357</fpage><lpage>2365</lpage><history><date date-type="received"><day>November</day>	<month>15,</month>	<year>2016</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>December</month>	<year>20,</year>	</date><date date-type="accepted"><day>December</day>	<month>23,</month>	<year>2016</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>
 
 
   Recent observations of Dwarf Satellite Galaxies (DSG) show that they have a clear tendency to stay in particular planes. Explanations with standard physics remain controversial. Recently, I proposed a new explanation of the galactic flat rotation curves, introducing a new cosmic acceleration due to expansion. In this paper, I apply this new acceleration to the dynamics of DSG’s (without dark matter). I show that this new acceleration implies planar structures for the DSG trajectories. More generally, it is shown that this acceleration produces a space structuration around any massive center. It remains a candidate to explain several cosmic observations without dark matter. 
 
</p></abstract><kwd-group><kwd>Dwarf Satellite Galaxies</kwd><kwd> Dark Matter</kwd><kwd> Expansion</kwd><kwd> Flat Rotation Curves</kwd><kwd> Galaxies</kwd><kwd>  Structure</kwd><kwd> Gravitation</kwd><kwd> Symmetry</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Dwarf Satellite Galaxies (DSG) have been discovered in the vicinity of Milky Way, M31 [<xref ref-type="bibr" rid="scirp.72940-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.72940-ref7">7</xref>] and also near low redshift galaxies [<xref ref-type="bibr" rid="scirp.72940-ref8">8</xref>] . Recent observations have shown that these DSG and other globular clusters tend to stay in thin plane structures [<xref ref-type="bibr" rid="scirp.72940-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref10">10</xref>] , which seem to be co-rotating with the host galaxy [<xref ref-type="bibr" rid="scirp.72940-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref12">12</xref>] . Most of these are orthogonal to the galactic plane, but some have been found with different angles [<xref ref-type="bibr" rid="scirp.72940-ref11">11</xref>] . In any case, they are clearly not isotropically distributed, and correlations are widespread [<xref ref-type="bibr" rid="scirp.72940-ref11">11</xref>] .</p><p>Several attempts have been made to explain these observations, introducing tidal effects [<xref ref-type="bibr" rid="scirp.72940-ref11">11</xref>] , past accretion processes [<xref ref-type="bibr" rid="scirp.72940-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref12">12</xref>] , etc. But for several others, these observations seem to be inconsistent with the expected distributions deduced from classical standard cosmological models [<xref ref-type="bibr" rid="scirp.72940-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref15">15</xref>] . More precisely, the assumption of quasi spherical Dark Matter (DM) around galaxies implies the presence of hundreds of DSG’s which should be isotropically distributed around large galaxies. This is in conflict with observations. Other proposals have also been imagined, such as DM haloes, filaments or “superhighways” [<xref ref-type="bibr" rid="scirp.72940-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref17">17</xref>] to attempt to answer the question. But is-it not too ad-hoc to suppose linear DM structures having similar patterns than the observed patterns to be explained?</p><p>The problem has also been addressed without Dark Matter by the MOND theory [<xref ref-type="bibr" rid="scirp.72940-ref15">15</xref>] .</p><p>I propose here a new attempt to provide a model without DM.</p></sec><sec id="s2"><title>2. Method</title><p>In a recent paper [<xref ref-type="bibr" rid="scirp.72940-ref18">18</xref>] , I have introduced a new Expansion Cosmic Acceleration (ECA) to explain the galactic flat rotation curves. This acceleration is proportional to the local expansion rate and to the velocity:</p><disp-formula id="scirp.72940-formula3"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x2.png"  xlink:type="simple"/></disp-formula><p>Then I showed [<xref ref-type="bibr" rid="scirp.72940-ref19">19</xref>] that this acceleration can be seen as a consequence of a rest-mass erosion theory, where space, time and mass are inter-dependent. It can also be considered as a consequence of SEC theory [<xref ref-type="bibr" rid="scirp.72940-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.72940-ref21">21</xref>] .</p><p>In the present paper, acceleration (1) is supposed to be applied to dwarf galaxies of a given host-galaxy. Solving the dynamics equations with this additional acceleration will give the DSG trajectories. It will then be seen that they remain in co-rotating thin plane structures. Finally, space structuration will be shown to result from the fundamental consequence of the ECA hypothesis, and is no more due to assumed DM structures.</p></sec><sec id="s3"><title>3. The Dynamics Equations</title><p>Let-us choose a classical 3D coordinate system, with the host (plane) galaxy centered in the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x3.png" xlink:type="simple"/></inline-formula> plane.</p><p>The velocity of a DSG located in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x4.png" xlink:type="simple"/></inline-formula> is made of three components (<xref ref-type="fig" rid="fig1">Figure 1</xref>):</p><p>-radial component: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x5.png" xlink:type="simple"/></inline-formula></p><p>-z-axial rotation:</p><disp-formula id="scirp.72940-formula4"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x6.png"  xlink:type="simple"/></disp-formula><p>-transverse rotation:</p><disp-formula id="scirp.72940-formula5"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x7.png"  xlink:type="simple"/></disp-formula><p>Then the well-known 3D dynamics equations can be written, for a DSG submitted to both Newtonian gravitation and to the cosmic acceleration (1):</p><disp-formula id="scirp.72940-formula6"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x8.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.72940-formula7"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x9.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.72940-formula8"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x10.png"  xlink:type="simple"/></disp-formula><p>The DSG is supposed to be far away from the center of the host galaxy and the total mass M, up to radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x11.png" xlink:type="simple"/></inline-formula>, is approximately constant. Furthermore, attraction forces from other DSG’s are neglected here.</p><p>Obviously, the purely Newtonian equations (without the last terms in (4), (5) and (6)) lead to the classical elliptic orbits, with no reason to stay in single planar structures.</p><p>With the cosmic acceleration terms, Equations (5) and (6) can be rewritten as:</p><disp-formula id="scirp.72940-formula9"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x12.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.72940-formula10"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x13.png"  xlink:type="simple"/></disp-formula><p>We then observe that:</p><disp-formula id="scirp.72940-formula11"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x14.png"  xlink:type="simple"/></disp-formula><p>Or equivalently:</p><disp-formula id="scirp.72940-formula12"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x15.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x16.png" xlink:type="simple"/></inline-formula> is constant.</p><p>Consequently, Equation (4) can be rewritten as:</p><disp-formula id="scirp.72940-formula13"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x17.png"  xlink:type="simple"/></disp-formula><p>This equation has the same form as the corresponding eq. for the trajectory of a star within the host galaxy plane, due to gravity and cosmic acceleration [<xref ref-type="bibr" rid="scirp.72940-ref18">18</xref>] . This “inside host-galaxy” case can be considered as a particular case of (11) when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x18.png" xlink:type="simple"/></inline-formula> or <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x19.png" xlink:type="simple"/></inline-formula> the flat rotation curve velocity.</p><p>More generally, from (10), the two components of the constant velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x20.png" xlink:type="simple"/></inline-formula> depend on an angle<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x21.png" xlink:type="simple"/></inline-formula>, such that:</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title>A small satellite galaxy is represented as a point, with its velocity vectors (the host-galaxy is in the xy plane)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/11-7502990x22.png"/></fig><disp-formula id="scirp.72940-formula14"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x23.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.72940-formula15"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x24.png"  xlink:type="simple"/></disp-formula></sec><sec id="s4"><title>4. The DSG Trajectories</title><p>From (12), (13) and (2), (3):</p><disp-formula id="scirp.72940-formula16"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x25.png"  xlink:type="simple"/></disp-formula><p>Then, derivating (13) and using the two Equations (7):</p><disp-formula id="scirp.72940-formula17"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x26.png"  xlink:type="simple"/></disp-formula><p>The <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x27.png" xlink:type="simple"/></inline-formula> relationship can then be deduced from (12) and (3):</p><disp-formula id="scirp.72940-formula18"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x28.png"  xlink:type="simple"/></disp-formula><p>Whose integration leads to:</p><disp-formula id="scirp.72940-formula19"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x29.png"  xlink:type="simple"/></disp-formula><p>where C is a constant (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x30.png" xlink:type="simple"/></inline-formula>).</p><p>The <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x31.png" xlink:type="simple"/></inline-formula> evolution can also be related to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x32.png" xlink:type="simple"/></inline-formula>, from (15) and (17):</p><disp-formula id="scirp.72940-formula20"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x33.png"  xlink:type="simple"/></disp-formula><p>Let us introduce a constant k such that:</p><disp-formula id="scirp.72940-formula21"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x34.png"  xlink:type="simple"/></disp-formula><p>(18) can be integrated into:</p><disp-formula id="scirp.72940-formula22"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x35.png"  xlink:type="simple"/></disp-formula><p>where the integration constant has been chosen in such a way that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x36.png" xlink:type="simple"/></inline-formula> corresponds to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x37.png" xlink:type="simple"/></inline-formula></p><p>From (17) and (20), it is easy to obtain the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x38.png" xlink:type="simple"/></inline-formula> relationship:</p><disp-formula id="scirp.72940-formula23"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x39.png"  xlink:type="simple"/></disp-formula><p>And, using (19), we get:</p><disp-formula id="scirp.72940-formula24"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x40.png"  xlink:type="simple"/></disp-formula><p>Incidentally, we observe that not all angular values are valid. As an instance, we have:</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x41.png" xlink:type="simple"/></inline-formula>with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x42.png" xlink:type="simple"/></inline-formula> (23)</p></sec><sec id="s5"><title>5. The DSG Planar Structures</title><p>The Cartesian coordinates of a DSG are:</p><disp-formula id="scirp.72940-formula25"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x43.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.72940-formula26"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x44.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.72940-formula27"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x45.png"  xlink:type="simple"/></disp-formula><p>From (22), it can be immediately deduced:</p><disp-formula id="scirp.72940-formula28"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x46.png"  xlink:type="simple"/></disp-formula><p>Physically, Equation (27) means that the DSG’s stay in a plane, cutting the galaxy plane along Oy (<xref ref-type="fig" rid="fig2">Figure 2</xref>). Its apex lies in the xz plane, where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x47.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x48.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x49.png" xlink:type="simple"/></inline-formula> is maximum, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x50.png" xlink:type="simple"/></inline-formula> is minimum (Equations (22)-(23)). When the DSG crosses the galaxy plane in Oy, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x51.png" xlink:type="simple"/></inline-formula>is minimum, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x52.png" xlink:type="simple"/></inline-formula> is maximum.</p><p>It results that any DSG must have its apex in the same plane (xz), and it must cross the galactic plane along the same line (Oy). All DSG trajectory planes must cut the galactic plane in Oy.</p><p>In particular, two important cases can be considered, depending on the initial conditions:</p><p>1)<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x53.png" xlink:type="simple"/></inline-formula>.</p><p>In this case, from (17), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x54.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x55.png" xlink:type="simple"/></inline-formula>. This describes the case of a star in the</p><p>galactic plane. Then, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x56.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x57.png" xlink:type="simple"/></inline-formula> is the galactic flat rotation velocity.</p><p>2) C is small.</p><p>In this case, for a non-z coaxial trajectory (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x58.png" xlink:type="simple"/></inline-formula>), the angle α remains close to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x59.png" xlink:type="simple"/></inline-formula></p><p>according to Equation (17). Velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x60.png" xlink:type="simple"/></inline-formula> is much smaller than<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x61.png" xlink:type="simple"/></inline-formula>, and from (20), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x62.png" xlink:type="simple"/></inline-formula></p><p>is also approximately equal to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x63.png" xlink:type="simple"/></inline-formula>.</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> For a given C value, any DSG must stay in the plane Oyξ, where its velocities are shown, at apex and at intersection with the galaxy plane on Oy</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/11-7502990x64.png"/></fig><p>Clearly, from (27), the DSG stays in a plane, which is quasi-perpendicular to the galactic plane and intersects it along Oy.</p><p>An individual orbit is mainly driven by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x65.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x66.png" xlink:type="simple"/></inline-formula>, but the small <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x67.png" xlink:type="simple"/></inline-formula> velocity forces it to stay in a quasi-perpendicular plane to the host galaxy (Equation (27)).</p><p>Since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x68.png" xlink:type="simple"/></inline-formula> is much smaller than<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x69.png" xlink:type="simple"/></inline-formula>, the DSG will go thru the galactic plane. But the whole planar structure is seen to rotate with respect to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x70.png" xlink:type="simple"/></inline-formula> plane, with velocity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x71.png" xlink:type="simple"/></inline-formula>, which is the galactic flat rotation velocity : the quasi-planar structure is co-rotating with the host galaxy.</p><p>Finally, the DSG orbit parameters r and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x72.png" xlink:type="simple"/></inline-formula> can be deduced from (11), (3) and (17).</p><p>As an instance, in the case:</p><disp-formula id="scirp.72940-formula29"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x73.png"  xlink:type="simple"/></disp-formula><p>and if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x74.png" xlink:type="simple"/></inline-formula> is supposed not to depend explicitly on time, Equation (11) can be written</p><p>as:</p><disp-formula id="scirp.72940-formula30"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x75.png"  xlink:type="simple"/></disp-formula><p>and integrated into:</p><disp-formula id="scirp.72940-formula31"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x76.png"  xlink:type="simple"/></disp-formula><p>(only valid for large r and large t, according to (28)).</p><p>Then, from (3) and (13):</p><disp-formula id="scirp.72940-formula32"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x77.png"  xlink:type="simple"/></disp-formula><p>can be integrated, using Equations (17) and (19). In the simple case<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x78.png" xlink:type="simple"/></inline-formula>, we obtain :</p><disp-formula id="scirp.72940-formula33"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/11-7502990x79.png"  xlink:type="simple"/></disp-formula><p>which describes the falling motion of a DSG from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x80.png" xlink:type="simple"/></inline-formula> at time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x81.png" xlink:type="simple"/></inline-formula> to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x82.png" xlink:type="simple"/></inline-formula> at</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x83.png" xlink:type="simple"/></inline-formula>.</p><p>More generally, Equation (27) describes a couple of planes, whose orientations depend on the C value.</p><p>To resume, there are several situations, depending on the initial ratio<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x84.png" xlink:type="simple"/></inline-formula>.</p><p>If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x85.png" xlink:type="simple"/></inline-formula> predominates, a spiral z-rotation will pull down the DSG into the host galactic plane. If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x86.png" xlink:type="simple"/></inline-formula> predominates, the DSG will fall towards the galactic plane. In any case, it stays in the planar structure (27), which is co-rotating with the galaxy at velocity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x87.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s6"><title>6. Discussion</title><p>If we recall that the host-galaxy mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x88.png" xlink:type="simple"/></inline-formula> has been considered to be constant (for large r), the whole preceding development is the same “as if”’ the whole galactic mass M had been concentrated in its center. Then the question arises why preferential planar structures do happen? They do not happen in the purely Newtonian case.</p><p>In fact, introducing a cosmic force proportional to velocity creates a symmetry break (<xref ref-type="fig" rid="fig3">Figure 3</xref>).</p><p>The figure made of a probe mass m at a distance r from a centered mass M is highly symmetrical. But, when the velocity vector of m is added, the new figure is modified under planar symmetry: the probe mass does not turn in the same direction any more. (In the above development, changing <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x89.png" xlink:type="simple"/></inline-formula> into <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x90.png" xlink:type="simple"/></inline-formula> needs <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x91.png" xlink:type="simple"/></inline-formula> to be changed into<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x92.png" xlink:type="simple"/></inline-formula>,as shown by Equations (15) or (31)).</p><p>This symmetry break does not allow any motion: it tends to give a structure to space (planar structures as described by Equation (27), and forbidden orientations such as (23)).</p><p>This conclusion is not only valid for planar host-galaxies, but for any massive attractive center. Consequently, our developments could be applied to any “small” massive objects in the vicinity of a huge massive center.</p><p>In this case, space structuration due to ECA can be seen in another way (<xref ref-type="fig" rid="fig4">Figure 4</xref>). Starting from a given unique massive center M placed at the point O, if a small probe mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x93.png" xlink:type="simple"/></inline-formula> is added, with velocity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x94.png" xlink:type="simple"/></inline-formula>, its trajectory will stay in the plane<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x95.png" xlink:type="simple"/></inline-formula>. A second probe mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x96.png" xlink:type="simple"/></inline-formula>, with another velocity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x97.png" xlink:type="simple"/></inline-formula>, will stay in plane<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x97.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x98.png" xlink:type="simple"/></inline-formula>. These two planes intersect along a straight line D. Any further probe mass planar trajectory is no more allowed: all other orbit planes must include D.</p><p>Since planar structures are predicted in the vicinity of one “host” massive center, linear filaments (2 plane intersects) should be obtained around two massive centers. And in the vicinity of more than two hosts, matter accumulation in spots should happen (plane and line intersect). Could it be that the new ECA give some insight to the structure of the universe at larger scales?</p><p>In any case, the ECA hypothesis engraves a fundamental structuration into space. Whenever, for the DM hypothesis, this structuration had to be assumed to come from the DM repartition itself.</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Symmetry break due to the cosmic acceleration. Left: Newtonian gravity is highly symmetrical. Right: with the additional cosmic force proportional to velocity, the mass probe and its image do not turn the same way</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/11-7502990x99.png"/></fig><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Space structuration around a massive spot: the orbit plane of the 3<sup>rd</sup> mass does necessarily include the intersection (D) of the two first orbit planes</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/11-7502990x100.png"/></fig></sec><sec id="s7"><title>7. Conclusions</title><p>I have shown that the hypothesis of the new cosmic acceleration (1) not only explains the flat rotation curve problem, but also leads to the conclusion that the DSG’s do stay in co-rotating planes with the host galaxy. Whenever their “falling down” velocity (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/11-7502990x101.png" xlink:type="simple"/></inline-formula>) is large, the planar structure is quasi-perpendicular to the host galaxy plane. This seems to be in correct agreement with most observations.</p><p>More generally, I have shown that the cosmic acceleration proportional to velocity introduces a symmetry break around any massive spot. This implies the formation of planar, linear or concentrated mass repartitions in space.</p><p>Of course, further observations and experiments will be needed to test the ECA hypothesis.</p><p>Close observations of DSG planes will have to be correlated with the proposed model. I also suggest introducing ECA into simulations of galaxy formation, galaxy collisions and also higher-level universe structures.</p></sec><sec id="s8"><title>Cite this paper</title><p>Fleuret, J. (2016) New Expansion Dynamics Applied to the Planar Structures of Satellite Galaxies and Space Structuration. Journal of Modern Phy- sics, 7, 2357-2365. http://dx.doi.org/10.4236/jmp.2016.716204</p></sec><sec id="s9"><title>Abbreviations</title><p>ECA = Expansion Cosmic Acceleration</p><p>DSG = Dwarf Satellite Galaxy</p><p>DM = Dark Matter</p></sec></body><back><ref-list><title>References</title><ref id="scirp.72940-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Libeskind, N.I., et al. (2011) Monthly Notices of the Royal Astronomical Society, 411, 1525. https://doi.org/10.1111/j.1365-2966.2010.17786.x</mixed-citation></ref><ref id="scirp.72940-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Libeskind, N.I., et al. 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