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Asymmetric dark matter theories generically allow for mass terms that lead to particle-antiparticle mixing. Over the age of the Universe, dark matter can thus oscillate from a purely asymmetric configuration into a symmetric mix of…

高能物理 - 唯象学 · 物理学 2013-05-30 Matthew R. Buckley , Stefano Profumo

The standard cold dark matter (CDM) model predicts too many and too dense small structures. We consider an alternative model that the dark matter undergoes two-body decays with cosmological lifetime $\tau$ into only one type of massive…

宇宙学与河外天体物理 · 物理学 2015-11-04 Dalong Cheng , M. -C. Chu , Jiayu Tang

We study thermal production of dark matter (DM) in a realization of the minimal models of Ref.~\cite{Bonnefoy:2023afx}, where parity is used to solve the strong CP problem by transforming the entire Standard Model (SM) into a mirror copy.…

高能物理 - 唯象学 · 物理学 2024-04-01 Quentin Bonnefoy , Lawrence Hall , Claudio Andrea Manzari , Amara McCune , Christiane Scherb

Motivated by inflation, the theory of big-bang nucleosynthesis and the quest for a deeper understanding of the fundamental forces and particles, a very successful paradigm for the development of structure in the Universe has evolved. It…

天体物理学 · 物理学 2009-10-28 Scott Dodelson , Evalyn Gates , Michael S. Turner

This write--up gives a rather elementary introduction into particle physics aspects of the cosmological Dark Matter puzzle. A fairly comprehensive list of possible candidates is given; in each case the production mechanism and possible ways…

高能物理 - 唯象学 · 物理学 2009-10-31 Manuel Drees

The freeze-in mechanism describes the out-of-equilibrium production of dark matter (DM) particles via feeble couplings or non-renormalisable interactions with large suppression scales. In the latter case, predictions suffer from a strong…

高能物理 - 唯象学 · 物理学 2025-04-16 Cristina Benso , Felix Kahlhoefer , Henda Mansour

The standard cold dark matter cosmological model, while successful in explaining the observed large scale structure of the Universe, tends to overpredict structure on small scales. It has been proposed this problem may be alleviated in a…

高能物理 - 唯象学 · 物理学 2011-03-21 Nicole F. Bell , Ahmad J. Galea , Raymond R. Volkas

We explore the production of thermal dark matter (DM) candidates (WIMPs, SIMPs, ELDERs and Cannibals) during cosmic reheating. Assuming a general parametrization for the scaling of the inflaton energy density and the standard model (SM)…

高能物理 - 唯象学 · 物理学 2024-08-28 Nicolás Bernal , Kuldeep Deka , Marta Losada

We present a simple model of dark matter that can address astrophysical and cosmological puzzles across a wide range of scales. The model is an application of the Secretly Asymmetric Dark Matter mechanism, where several flavors of dark…

高能物理 - 唯象学 · 物理学 2019-08-15 Christopher Dessert , Can Kilic , Cynthia Trendafilova , Yuhsin Tsai

We discuss a supersymmetric model for cogenesis of dark and baryonic matter where the dark matter (DM) has mass in the 8-10 GeV range as indicated by several direct detection searches including most recently the CDMS experiment with the…

高能物理 - 唯象学 · 物理学 2015-06-15 Rouzbeh Allahverdi , Bhaskar Dutta , Rabindra N. Mohapatra , Kuver Sinha

We consider thermal production mechanisms of self-interacting dark matter in models with gauged $Z_3$ symmetry. A complex scalar dark matter is stabilized by the $Z_3$, that is the remnant of a local dark $U(1)_d$. Light dark matter with…

高能物理 - 唯象学 · 物理学 2017-02-01 Soo-Min Choi , Yoo-Jin Kang , Hyun Min Lee

Recently it was shown that dark matter with mass of order the weak scale can be charged under a new long-range force, decoupled from the Standard Model, with only weak constraints from early Universe cosmology. Here we consider the…

宇宙学与河外天体物理 · 物理学 2017-08-30 Prateek Agrawal , Francis-Yan Cyr-Racine , Lisa Randall , Jakub Scholtz

We suggest that an interplay between microscopic and macroscopic physics can give rise to dark matter (DM) whose interactions with the visible sector fundamentally undulate in time, independent of celestial dynamics. A concrete example is…

高能物理 - 唯象学 · 物理学 2020-12-30 Joe Davighi , Matthew McCullough , Joseph Tooby-Smith

Atomic dark matter is a simple but highly theoretically motivated possibility for an interacting dark sector that could constitute some or all of dark matter. We perform a comprehensive study of precision cosmological observables on minimal…

高能物理 - 唯象学 · 物理学 2023-07-31 Saurabh Bansal , Jared Barron , David Curtin , Yuhsin Tsai

From the particle physics point of view, the most peculiar property of the dark matter particle is its stability on cosmological time scales. We briefly review the possible origins of this characteristic feature for candidates whose relic…

高能物理 - 唯象学 · 物理学 2010-12-22 Thomas Hambye

We present a class of dark matter models, in which the dark matter particle is a feebly interacting massive particle (FIMP) produced via the decay of an electrically charged and/or colored parent particle. Given the feeble interaction, dark…

高能物理 - 唯象学 · 物理学 2019-10-02 G. Bélanger , N. Desai , A. Goudelis , J. Harz , A. Lessa , J. M. No , A. Pukhov , S. Sekmen , D. Sengupta , B. Zaldivar , J. Zurita

It is now believed that the universe is composed of a small amount of the normal luminous matter, a substantial amount of matter (Cold Dark Matter: CDM) which is non-luminous and a large amount of smooth energy (Dark Energy: DE). Both CDM…

This theoretical particle physics thesis is an investigation into old and new symmetries of Nature. Known symmetries and conservation laws serve as a guide for dark and visible sector model building. New symmetries of Nature are proposed,…

高能物理 - 唯象学 · 物理学 2020-01-03 Jennifer Rittenhouse West

The kinetic decoupling of weakly interacting massive particles (WIMPs) in the early universe sets a scale that can directly be translated into a small-scale cutoff in the spectrum of matter density fluctuations. The formalism presented here…

宇宙学与河外天体物理 · 物理学 2014-11-18 Torsten Bringmann

Warm dark matter cosmologies have been widely studied as an alternative to the cold dark matter paradigm, the characteristic feature being a suppression of structure formation on small cosmological scales. A very similar situation occurs if…

高能物理 - 唯象学 · 物理学 2016-12-02 Torsten Bringmann , Haavard Tveit Ihle , Joern Kersten , Parampreet Walia