Unified Dark Matter Scalar Field Models

<table>The redshift evolution of the scalar field equation of state parameter <svg height="11.9875" id="M579" style="vertical-align:-3.4098pt" version="1.1" viewbox="0 0 40.775002 11.9875" width="40.775002" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
<g transform="matrix(.017,-0,0,-.017,.062,7.675)"><path d="M689 332q0 -81 -40 -161.5t-103.5 -131.5t-127.5 -51q-32 0 -58.5 16t-40.5 46q-70 -62 -139 -62q-45 0 -77.5 30t-32.5 86q0 8 7 52q11 77 45 187q6 19 6 34q0 6 -7 6q-24 0 -78 -64l-20 23q32 48 73 77t78 29q32 0 32 -43q0 -30 -12 -73q-27 -95 -38 -152
q-8 -44 -8 -58q0 -77 68 -77q31 0 60 33.5t39 77.5l62 260l75 16l5 -6l-63 -246q-8 -29 -8 -58q0 -77 68 -77q66 0 116 75.5t50 194.5q0 43 -12 57q-11 12 -11 24q0 19 15 35.5t34 16.5q18 0 30.5 -34.5t12.5 -81.5z" id="x1D464"></path></g>
<g transform="matrix(.012,-0,0,-.012,12.162,11.762)"><path d="M716 650v-28q-46 -3 -65 -15.5t-22 -43.5q-6 -54 -6 -162v-82q0 -184 -75 -264q-68 -69 -180 -69q-98 0 -160 48q-88 67 -88 238v249q0 66 -13.5 81t-73.5 20v28h258v-28q-59 -4 -72.5 -19t-13.5 -82v-227q0 -122 48 -188t140 -66q189 0 189 286v75q0 111 -7 165
q-4 29 -24 40.5t-73 15.5v28h238z" id="x55"></path></g><g transform="matrix(.012,-0,0,-.012,20.92,11.762)"><path d="M43 650h280q194 0 282 -85q85 -82 85 -215q0 -173 -123 -267q-107 -83 -297 -83h-236v27q65 5 79.5 19.5t14.5 77.5v402q0 45 -6 62.5t-21.5 24t-57.5 9.5v28zM213 547v-416q0 -55 24.5 -75t81.5 -20q133 0 203 86t70 214q0 80 -30 143t-88 97q-66 41 -170 41
q-62 0 -78 -13q-13 -9 -13 -57z" id="x44"></path></g><g transform="matrix(.012,-0,0,-.012,29.499,11.762)"><path d="M861 0h-263v28q61 5 73 22t12 97l-4 408h-4l-244 -548h-20l-224 534h-2l-15 -285q-5 -98 -3 -166q1 -34 19.5 -45t72.5 -17v-28h-233v28q45 5 62.5 17t22.5 43q11 65 19 183l14 208q3 36 3.5 55t-2.5 37.5t-6.5 25t-16.5 13t-25.5 8t-39.5 4.5v28h164l228 -501l232 501
h170v-28q-68 -6 -81 -21.5t-11 -91.5l9 -362q2 -80 15 -97t78 -22v-28z" id="x4D"></path></g>
</svg> (continuous line) is compared with that of the sum of the DM + DE components in a standard <svg height="11.425" id="M580" style="vertical-align:-0.0pt" version="1.1" viewbox="0 0 11.7875 11.425" width="11.7875" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
<g transform="matrix(.017,-0,0,-.017,.062,11.363)"><path d="M671 0h-247v28q49 7 60 18.5t0 45.5l-155 438h-2q-21 -61 -74 -204.5t-75 -210.5q-15 -51 -4.5 -65t67.5 -22v-28h-221v28q50 9 69 26.5t45 84.5l202 517l32 9l194 -535q23 -61 42 -78.5t67 -23.5v-28z" id="x39B"></path></g>
</svg>CDM model (dashed line); see [<a href="/journals/aa/2010/904379/#B33">33</a>].</table>

Advances in Astronomy

Unified Dark Matter Scalar Field Models

Figure 3