Exploring the self interacting dark matter properties from low redshift observations
Abstract We calculate the shear ( $$\eta $$ η ) and bulk viscosity ( $$\zeta $$ ζ ) of Self Interacting Dark Matter (SIDM) fluid using the kinetic theory formalism. Using the astrophysical constraints on dark matter self-interaction cross section over mass $$ \sigma /m $$ σ / m , we demonstrate that...
I tiakina i:
| Kaituhi matua: | |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
SpringerOpen
2022-11-01
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| Rangatū: | European Physical Journal C: Particles and Fields |
| Urunga tuihono: | https://doi.org/10.1140/epjc/s10052-022-10907-8 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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