The Logotropic Dark Fluid as a unification of dark matter and dark energy

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• 作者：Pierre-Henri Chavanis ^{chavanis@irsamc.ups-tlse.fr" class="auth_mail" title="E-mail the corresponding author}
• 刊名：Physics Letters B
• 出版年：2016
• 出版时间：10 July 2016
• 年：2016
• 卷：758
• 期：Complete
• 页码：59-66
• 全文大小：497 K

文摘

We propose a heuristic unification of dark matter and dark energy in terms of a single “dark fluid” with a logotropic equation of state g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si1.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=d6bae1c67c463a2fee746908ffa2e09e" title="Click to view the MathML source">P=Aln⁡(ρ/ρ_P)gif" overflow="scroll">P=Aln⁡(ρ/ρP), where ρ   is the rest-mass density, g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si2.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=c23014b8ba06f16b83c5b8d77f295aa3">g class="imgLazyJSB inlineImage" height="16" width="144" alt="View the MathML source" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316301150-si2.gif">gif" overflow="scroll">ρP=5.16×1099gm−3 is the Planck density, and A is the logotropic temperature. The energy density ϵ   is the sum of a rest-mass energy term g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si3.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=392d259dfbbf126ad944f4948424fb28" title="Click to view the MathML source">ρc²∝a⁻³gif" overflow="scroll">ρc2∝a−3 mimicking dark matter and an internal energy term g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si4.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=802f07233221c69e99bdf6999723cb8a" title="Click to view the MathML source">u(ρ)=−P(ρ)−A=3Aln⁡a+Cgif" overflow="scroll">u(ρ)=−P(ρ)−A=3Aln⁡a+C mimicking dark energy (a   is the scale factor). The logotropic temperature is approximately given by g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si5.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=ca80c7bea1c6825e4c505dc44c9ea515" title="Click to view the MathML source">A≃ρ_Λc²/ln⁡(ρ_P/ρ_Λ)≃ρ_Λc²/[123ln⁡(10)]gif" overflow="scroll">A≃ρΛc2/ln⁡(ρP/ρΛ)≃ρΛc2/[123ln⁡(10)], where g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si6.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=e6ddfc8ca7e7bd9ffa9fbc1e46589eda">g class="imgLazyJSB inlineImage" height="16" width="154" alt="View the MathML source" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316301150-si6.gif">gif" overflow="scroll">ρΛ=6.72×10−24gm−3 is the cosmological density and 123 is the famous number appearing in the ratio g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si7.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=5337850b9f67bc425c5f28ac5fde3cd8" title="Click to view the MathML source">ρ_P/ρ_Λ∼10¹²³gif" overflow="scroll">ρP/ρΛ∼10123 between the Planck density and the cosmological density. More precisely, we obtain g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si238.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=93d6e79a077d5792740e61f565af11a1">g class="imgLazyJSB inlineImage" height="16" width="164" alt="View the MathML source" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316301150-si238.gif">gif" overflow="scroll">A=2.13×10−9gm−1s−2 that we interpret as a fundamental constant. At the cosmological scale, our model fulfills the same observational constraints as the ΛCDM model (they will differ in about 25 Gyrs when the logotropic universe becomes phantom). However, the logotropic dark fluid has a nonzero speed of sound and a nonzero Jeans length which, at the beginning of the matter era, is about g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si9.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=120f90774c69760a6d8ff216890adc72">g class="imgLazyJSB inlineImage" height="14" width="79" alt="View the MathML source" style="margin-top: -5px; vertical-align: middle" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316301150-si9.gif">gif" overflow="scroll">λJ=40.4pc, in agreement with the minimum size of the dark matter halos observed in the universe. The existence of a nonzero Jeans length may solve the missing satellite problem. At the galactic scale, the logotropic pressure balances the gravitational attraction, providing halo cores instead of cusps. This may solve the cusp problem. The logotropic equation of state generates a universal rotation curve that agrees with the empirical Burkert profile of dark matter halos up to the halo radius. In addition, it implies that all the dark matter halos have the same surface density g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si10.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=a00e5f11fc67b0b31d5c92afd8002664">g class="imgLazyJSB inlineImage" height="16" width="155" alt="View the MathML source" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316301150-si10.gif">gif" overflow="scroll">Σ0=ρ0rh=141M⊙/pc2 and that the mass of dwarf galaxies enclosed within a sphere of fixed radius g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si11.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=5eb7aeaa26808f0e12b69a78b41a6546">g class="imgLazyJSB inlineImage" height="13" width="72" alt="View the MathML source" style="margin-top: -5px; vertical-align: middle" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316301150-si11.gif">gif" overflow="scroll">ru=300pc has the same value g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si12.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=8a2ebf3b2387d8ab8254058700ff5ef8">g class="imgLazyJSB inlineImage" height="16" width="140" alt="View the MathML source" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316301150-si12.gif">gif" overflow="scroll">M300=1.93×107M⊙, in remarkable agreement with the observations [Donato et al. [10], Strigari et al. [13]]. It also implies the Tully–Fisher relation g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316301150&_mathId=si13.gif&_user=111111111&_pii=S0370269316301150&_rdoc=1&_issn=03702693&md5=57d5a777a78ef08a366a9738e271b3ba">g class="imgLazyJSB inlineImage" height="19" width="151" alt="View the MathML source" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316301150-si13.gif">gif" overflow="scroll">Mb/vh4=44M⊙km−4s4. We stress that our model has no free parameter.