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相关论文: Free streaming in mixed dark matter

200 篇论文

In this paper, we propose the sterile neutrino portal dark matter in $\nu$THDM. This model can naturally generate tiny neutrino mass with the neutrinophilic scalar doublet $\Phi_{\nu}$ and sterile neutrinos $N$ around TeV scale. Charged…

高能物理 - 唯象学 · 物理学 2023-06-07 Ang Liu , Feng-Lan Shao , Zhi-Long Han , Yi Jin , Honglei Li

We explore a model for a fermionic dark matter particle family which decouples from the rest of the partices when at least all standard model particles are in equilibrium. We calculate the allowed ranges for mass and chemical potential to…

天体物理学 · 物理学 2008-11-26 T. Boeckel , J. Schaffner-Bielich

If dark matter (DM) is millicharged or darkly charged, collective plasma processes may dominate momentum exchange over direct particle collisions. Plasma streaming instabilities can couple the momentum of the DM to counter-streaming baryons…

宇宙学与河外天体物理 · 物理学 2023-04-19 Akaxia Cruz , Matthew McQuinn

We present updated constraints on the free-streaming nature of cosmological neutrinos from cosmic microwave background (CMB) power spectra, baryonic acoustic oscillation data, and local measurements of the Hubble constant. Specifically, we…

宇宙学与河外天体物理 · 物理学 2018-01-22 Lachlan Lancaster , Francis-Yan Cyr-Racine , Lloyd Knox , Zhen Pan

The free streaming length of dark matter particles determines the abundance of structure on sub-galactic scales. We present a statistical technique, amendable to any parameterization of subhalo density profile and mass function, to probe…

宇宙学与河外天体物理 · 物理学 2018-08-29 Daniel Gilman , Simon Birrer , Tommaso Treu , Charles R. Keeton , Anna Nierenberg

The clustering properties of sterile neutrinos are studied within an extension of the minimal standard model, where these are produced via the decay of a gauge singlet scalar. The distribution function after decoupling is strongly out of…

天体物理学 · 物理学 2008-12-18 D. Boyanovsky

We provide a semi-analytic study of the small scale aspects of the power spectra of warm dark matter (WDM) candidates that decoupled while relativistic with arbitrary distribution functions. These are characterized by two widely different…

宇宙学与河外天体物理 · 物理学 2011-03-23 Daniel Boyanovsky , Jun Wu

If dark matter has even been in sufficient thermal contact with the visible sector and sufficiently light ($m_\chi\lesssim\mathcal{O}(10)~\text{keV}$), the thermal motion inherited from the visible sector will cause significant free…

高能物理 - 唯象学 · 物理学 2019-10-02 Ran Huo , Tao Xu

We present updated constraints on the free-streaming of warm dark matter (WDM) particles derived from an analysis of the Lya flux power spectrum measured from high-resolution spectra of 25 z > 4 quasars obtained with the Keck High…

宇宙学与河外天体物理 · 物理学 2015-06-16 M. Viel , G. D. Becker , J. S. Bolton , M. G. Haehnelt

We study how present data probe standard and non-standard properties of neutrinos and the possible existence of new light particles, freely-streaming or interacting, among themselves or with neutrinos. Our results include: sum m_nu < 0.40…

天体物理学 · 物理学 2009-11-11 Marco Cirelli , Alessandro Strumia

I consider constraints from observations on a cutoff scale in clustering due to free streaming of the dark matter in a warm dark matter cosmological model with a cosmological constant. The limits are derived in the framework of a sterile…

天体物理学 · 物理学 2007-05-23 Kevork Abazajian

We perform a set of cosmological simulations of structure formation in a mixed dark matter (MDM) model. Our model is motivated by the recently identified $3.5\,{\rm keV}$ X-ray line, which can be explained by the decay of non-resonantly…

宇宙学与河外天体物理 · 物理学 2016-01-21 Akira Harada , Ayuki Kamada

Dark Matter (DM) is generally assumed to be massive, cold and collisionless from the structure formation point of view. A more correct statement however is that DM indeed experiences collisional damping, but on a scale which is supposed to…

天体物理学 · 物理学 2007-05-23 C. Boehm , H. Mathis , J. Devriendt , J. Silk

We present a new dark matter model BDM which is an hybrid between hot dark matter HDM and cold dark matter CDM, in which the BDM particles behave as HDM above the energy scale E_c and as CDM below this scale. Evolution of structure…

宇宙学与河外天体物理 · 物理学 2015-05-13 Axel de la Macorra

The matter power spectrum at comoving scales of (1-40) h^{-1} Mpc is very sensitive to the presence of Warm Dark Matter (WDM) particles with large free streaming lengths. We present constraints on the mass of WDM particles from a combined…

天体物理学 · 物理学 2009-11-10 M. Viel , J. Lesgourgues , M. G. Haehnelt , S. Matarrese , A. Riotto

Cosmological simulations for cold dark matter (DM) indicate that a large number of streams might exist in our Galaxy. The present work incorporates gravitational focusing (GF) effects on streaming DM constituents by the Sun and the Earth…

天体物理仪器与方法 · 物理学 2023-12-06 Abaz Kryemadhi , Marios Maroudas , Andreas Mastronikolis , Konstantin Zioutas

Stellar streams are remnants of globular clusters or dwarf galaxies that have been tidally disrupted by the gravitational potential of their host galaxy. Streams originating from dwarfs can be particularly compelling targets for indirect…

高能天体物理现象 · 物理学 2025-02-24 Cristina Fernandez-Suarez , Miguel A. Sanchez-Conde

We propose a multi-messenger frontier probe of non-thermal or freeze-in massive particle (FIMP) dark matter (DM) by considering an effective field theory (EFT) setup. Assuming leptophilic operators connecting DM with the standard model (SM)…

高能物理 - 唯象学 · 物理学 2025-11-13 Debasish Borah , Nayan Das , Sahabub Jahedi , Dipankar Pradhan

We consider cosmology of the recently introduced mimetic matter with higher derivatives (HD). Without HD this system describes irrotational dust - Dark Matter (DM) as we see it on cosmologically large scales. DM particles correspond to the…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Leila Mirzagholi , Alexander Vikman

We present new measurements of the free-streaming of warm dark matter (WDM) from Lyman-$\alpha$ flux-power spectra. We use data from the medium resolution, intermediate redshift XQ-100 sample observed with the X-shooter spectrograph ($z=3 -…