Hypothetical form of dark matter
Inastrophysics andparticle physics ,self-interacting dark matter (SIDM ) is an alternative class ofdark matter particles that have strong interactions, in contrast to the standardcold dark matter model (CDM). SIDM was postulated in 2000[ 1] as a solution to thecore-cusp problem .[ 2] [ 3] [ 4] In the simplest models of DM self-interactions, a Yukawa-type potential and a force carrierφ mediates between two dark matter particles.[ 5] On galactic scales, DM self-interaction leads to energy and momentum exchange between DM particles. Over cosmological time scales this results in isothermal cores in the central region of dark matter haloes.
If the self-interacting dark matter is inhydrostatic equilibrium , its pressure and density follow:
∇ P χ / ρ χ = ∇ Φ tot = ∇ ( Φ χ + Φ b ) , {\displaystyle \nabla P_{\chi }/\rho _{\chi }=\nabla \Phi _{\text{tot}}=\nabla (\Phi _{\chi }+\Phi _{\text{b}}),} whereΦ χ {\displaystyle \Phi _{\chi }} andΦ b {\displaystyle \Phi _{\text{b}}} are the gravitational potential of the dark matter and a baryon respectively. The equation naturally correlates the dark matter distribution to that of the baryonic matter distribution. With this correlation, the self-interacting dark matter can explain phenomena such as theTully–Fisher relation .
Self-interacting dark matter has also been postulated as an explanation for theDAMA annual modulation signal.[ 6] [ 7] [ 8] Moreover, it is shown that it can serve the seed ofsupermassive black holes at high redshift.[ 9] SIDM may have originated in a so-called "Dark Big Bang ".[ 10]
In July 2024 a study proposed SIDM solves the "final-parsec problem ",[ 11] [ 12] two months later another study proposed the same withfuzzy cold dark matter .[ 13] [ 14]
^ Spergel, David N.; Steinhardt, Paul J. (April 2000)."Observational Evidence for Self-Interacting Cold Dark Matter" .Physical Review Letters .84 (17):3760– 3763.arXiv :astro-ph/9909386 .Bibcode :2000PhRvL..84.3760S .doi :10.1103/PhysRevLett.84.3760 .ISSN 0031-9007 .PMID 11019199 .S2CID 6669358 . ^ Moore, Ben (August 1994)."Evidence against dissipation-less dark matter from observations of galaxy haloes" .Nature .370 (6491):629– 631.Bibcode :1994Natur.370..629M .doi :10.1038/370629a0 .ISSN 0028-0836 .S2CID 4325561 . ^ Oh, Se-Heon; de Blok, W. J. G.; Walter, Fabian; Brinks, Elias; Kennicutt, Robert C. (December 2008)."High-Resolution Dark Matter Density Profiles of THINGS Dwarf Galaxies: Correcting for Noncircular Motions" .The Astronomical Journal .136 (6):2761– 2781.arXiv :0810.2119 .Bibcode :2008AJ....136.2761O .doi :10.1088/0004-6256/136/6/2761 .ISSN 0004-6256 . ^ Oh, Se-Heon; Hunter, Deidre A.; Brinks, Elias; Elmegreen, Bruce G.; Schruba, Andreas; Walter, Fabian; Rupen, Michael P.; Young, Lisa M.; Simpson, Caroline E.; Johnson, Megan C.; Herrmann, Kimberly A. (June 2015)."High-resolution Mass Models of Dwarf Galaxies from LITTLE THINGS" .The Astronomical Journal .149 (6): 180.arXiv :1502.01281 .Bibcode :2015AJ....149..180O .doi :10.1088/0004-6256/149/6/180 .ISSN 0004-6256 . ^ Loeb, Abraham; Weiner, Neal (April 2011)."Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential" .Physical Review Letters .106 (17) 171302.arXiv :1011.6374 .Bibcode :2011PhRvL.106q1302L .doi :10.1103/PhysRevLett.106.171302 .ISSN 0031-9007 .PMID 21635025 . ^ Mitra, Saibal (15 June 2005). "Has DAMA detected self-interacting dark matter?".Physical Review D .71 (12) 121302.arXiv :astro-ph/0409121 .Bibcode :2005PhRvD..71l1302M .doi :10.1103/PhysRevD.71.121302 .S2CID 31554326 . ^ Moskowitz, Clara (20 April 2015)."Dark Matter May Feel a "Dark Force" That the Rest of the Universe Does Not" .Scientific American . ^ Richard Massey; et al. (June 2015)."The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827" .Monthly Notices of the Royal Astronomical Society .449 (4P):3393– 3406.arXiv :1504.03388 .Bibcode :2015MNRAS.449.3393M .doi :10.1093/mnras/stv467 . commentaryThe Possible First Signs of Self-interacting Dark Matter ^ Feng, W.-X.; Yu, H.-B.; Zhong, Y.-M. (2021)."Seeding Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons" .The Astrophysical Journal Letters .914 (2): L26.arXiv :2010.15132 .Bibcode :2021ApJ...914L..26F .doi :10.3847/2041-8213/ac04b0 . "How a supermassive black hole originates: Study points to a seed black hole produced by a dark matter halo collapse." ScienceDaily , 16 June 2021.^ "Dancing in the dark" .The Economist . 9 March 2024.^ Alonso-Álvarez, Gonzalo; Cline, James M.; Dewar, Caitlyn (2024-07-09)."Self-Interacting Dark Matter Solves the Final Parsec Problem of Supermassive Black Hole Mergers" .Physical Review Letters .133 (2) 021401.arXiv :2401.14450 .Bibcode :2024PhRvL.133b1401A .doi :10.1103/PhysRevLett.133.021401 .ISSN 0031-9007 .PMID 39073950 . ^ Jonathan Gilbert (2024-08-19)." 'Final parsec problem' that makes supermassive black holes impossible to explain could finally have a solution" .livescience.com . Retrieved2024-08-20 . ^ Koo, Hyeonmo; Bak, Dongsu; Park, Inkyu; Hong, Sungwook E.; Lee, Jae-Weon (September 2024)."Final parsec problem of black hole mergers and ultralight dark matter" .Physics Letters B .856 138908.arXiv :2311.03412 .Bibcode :2024PhLB..85638908K .doi :10.1016/j.physletb.2024.138908 . ^ O'Callaghan, Jonathan (2024-10-23)."How Do Merging Supermassive Black Holes Pass the Final Parsec?" .Quanta Magazine . Retrieved2024-10-24 .
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