Dark matter, density perturbations and structure formation

2; 3) ((1) Dipartimento di Matematica; A. Del Popolo (1; Istanbul; ITALY; (2) Feza Gursey Institute; Physics Department; Turkey); Turkey; (3) Bogazici University; Universita' Statale di Bergamo

Dark matter, density perturbations and structure formation

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arxiv astro-ph/0209128 v1 submitted 2002-09-07 astro-ph

A. Del Popolo (1 , 2 , 3) ((1) Dipartimento di Matematica , Universita' Statale di Bergamo , ITALY; (2) Feza Gursey Institute , Istanbul , Turkey; (3) Bogazici University , Physics Department

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keywords darkmattercomponentsdensityevolutionformationfundamentalorigin

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This paper provides a review of the variants of dark matter (CDM, HDM) which are thought to be fundamental components of the universe and their role in origin and evolution of structures.

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Constraints on dark matter self-interaction from velocity distribution function in isolated halos
hep-ph 2025-05 conditional novelty 6.0 of 10

N-body simulations and rotation-curve data constrain the dark matter self-interaction cross-section to σ/m ≤ 2.7 cm²/g at 95% C.L. for Milky Way-scale halos.

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