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相关论文: Evidence for dark matter modulation in CoGeNT?

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A convincing identification of dark matter (DM) particles can probably be achieved only through a combined analysis of different detections strategies, which provides an effective way of removing degeneracies in the parameter space of DM…

高能天体物理现象 · 物理学 2014-11-21 Pasquale D. Serpico , Gianfranco Bertone

I consider some of the issues we face in trying to understand dark energy. Huge fluctuations in the unknown dark energy equation of state can be hidden in distance data, so I argue that model-independent tests which signal if the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Chris Clarkson

This paper explores the possibility that dark matter particles are objects with a set of excitable levels, as for a string or drum. A change in excitation is associated with the absorption or emission of a photon, and the probability of…

宇宙学与河外天体物理 · 物理学 2020-02-25 Andrew J. Wren

Bayesian statistical methods offer a simple and consistent framework for incorporating uncertainties into a multi-parameter inference problem. In this work we apply these methods to a selection of current direct dark matter searches. We…

高能物理 - 唯象学 · 物理学 2015-05-28 Chiara Arina , Jan Hamann , Yvonne Y. Y. Wong

We revisit a cosmological model where dark matter (DM) and dark energy (DE) follow barotropic equations of state, allowing deviations from the standard $\Lambda$CDM framework (i.e. $w_{dm} \neq 0$, $w_{de} \neq -1$), considering both flat…

宇宙学与河外天体物理 · 物理学 2025-11-24 Dorian Araya , Cristian Castillo , Genly Leon , Juan Magaña , Angie Barr Domínguez , Miguel A. García-Aspeitia

We investigate the hypothesis that Coulomb-type interactions between dark matter (DM) and baryons explain the anomalously low 21cm brightness-temperature minimum at redshift z ~ 17 that was recently measured by the EDGES experiment. In…

宇宙学与河外天体物理 · 物理学 2018-12-05 Ely D. Kovetz , Vivian Poulin , Vera Gluscevic , Kimberly K. Boddy , Rennan Barkana , Marc Kamionkowski

To properly solve the coincidence problem ($\Omega_\mathrm{DM} \simeq 5\Omega_\mathrm{VM}$) in a model of asymmetric dark matter, one cannot simply relate the number densities of visible and dark matter without also relating their particle…

高能物理 - 唯象学 · 物理学 2024-04-10 Alexander C. Ritter , Raymond R. Volkas

In this article, we review a series of recent theoretical results regarding a conventional approach to the dark energy (DE) concept. This approach is distinguished among others for its simplicity and its physical relevance. By compromising…

宇宙学与河外天体物理 · 物理学 2016-04-20 Kostas Kleidis , Nikolaos K. Spyrou

Models with dark energy decaying into dark matter have been proposed to solve the coincidence problem in cosmology. We study the effect of such coupling in the matter power spectrum. Due to the interaction, the growth of matter density…

天体物理学 · 物理学 2008-11-26 G. Olivares , F. Atrio-Barandela , D. Pavon

The new Dark Energy Spectroscopic Instrument (DESI) DR2 results have strengthened the possibility that dark energy is dynamical, i.e., it has evolved over the history of the Universe. One simple, but theoretically well motivated and widely…

宇宙学与河外天体物理 · 物理学 2025-04-14 Yashar Akrami , George Alestas , Savvas Nesseris

I present a class of hidden sector dark matter (DM) models with local dark gauge symmetries, where DM is stable due to unbroken local dark gauge symmetry, or due topology, or it is long-lived because of some accidental symme- tries, and the…

高能物理 - 唯象学 · 物理学 2015-03-19 P. Ko

The velocity distribution function of dark matter particles is expected to show significant departures from a Maxwell-Boltzmann distribution. This can have profound effects on the predicted dark matter - nucleon scattering rates in direct…

星系天体物理 · 物理学 2014-11-20 M. Kuhlen , N. Weiner , J. Diemand , P. Madau , B. Moore , D. Potter , J. Stadel , M. Zemp

A new frontier in the search for dark matter (DM) is based on the idea of detecting the decoherence caused by DM scattering against a mesoscopic superposition of normal matter. Such superpositions are uniquely sensitive to very small…

量子物理 · 物理学 2017-08-02 C. Jess Riedel , Itay Yavin

The nature of dark energy can be probed not only through its equation of state, but also through its microphysics, characterized by the sound speed of perturbations to the dark energy density and pressure. As the sound speed drops below the…

宇宙学与河外天体物理 · 物理学 2010-05-25 Roland de Putter , Dragan Huterer , Eric V. Linder

While cold dark matter is widely supported by a range of cosmological observations, it encounters several difficulties at smaller scales. These issues have prompted the investigation of various alternative dark matter candidates, leaving…

宇宙学与河外天体物理 · 物理学 2025-07-23 Jian-Qi Liu , Yan-Hong Yao , Yan Su , Jia-Wei Wu

If dark matter (DM) simply consists in a scalar particle interacting dominantly with the Higgs boson, the ratio of its annihilation cross section ---which is relevant both for the relic abundance and indirect detection--- and its…

高能物理 - 唯象学 · 物理学 2014-11-20 Sarah Andreas , Chiara Arina , Thomas Hambye , Fu-Sin Ling , Michel H. G. Tytgat

Numerous theories extending beyond the standard model of particle physics predict the existence of bosons that could constitute the dark matter (DM) permeating the universe. In the standard halo model (SHM) of galactic dark matter the…

A large number of studies, all using Bayesian parameter inference from Markov Chain Monte Carlo methods, have constrained the presence of a decaying dark matter component. All such studies find a strong preference for either very long-lived…

宇宙学与河外天体物理 · 物理学 2022-11-04 Emil Brinch Holm , Laura Herold , Steen Hannestad , Andreas Nygaard , Thomas Tram

It is usually assumed that dark matter direct detection is sensitive to a large fraction of the dark matter (DM) velocity distribution. We propose an alternative form of dark matter-nucleus scattering which only probes a narrow range of DM…

高能物理 - 唯象学 · 物理学 2009-11-13 Yang Bai , Patrick J. Fox

We propose a novel strategy to search for new physics in timing spectra, envisioning the situation in which a new particle comes from the decay of its heavier partner with a finite particle width. The timing distribution of events induced…

高能物理 - 唯象学 · 物理学 2020-04-01 Bhaskar Dutta , Doojin Kim , Shu Liao , Jong-Chul Park , Seodong Shin , Louis E. Strigari