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We show that hidden hot dark matter, hidden-sector dark matter with interactions that decouple when it is relativistic, is a viable dark matter candidate provided it has never been in thermal equilibrium with the particles of the standard…

宇宙学与河外天体物理 · 物理学 2009-12-15 Kris Sigurdson

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

The relic abundance of thermal dark matter particles is generally assumed to be inversely proportional to their annihilation rate, which is therefore constrained by the present matter density, <sigma v> ~ 10^{-26} Omega_{dm}^{-1} cm^3…

宇宙学与河外天体物理 · 物理学 2010-01-07 Leonid Chuzhoy

Matter in neutron star collisions can reach densities up to few times the nuclear saturation threshold and temperatures up to one hundred MeV. Understanding the structure and composition of such matter requires many-body nonperturbative…

广义相对论与量子宇宙学 · 物理学 2019-09-04 Albino Perego , Sebastiano Bernuzzi , David Radice

The secluded dark matter resides within a hidden sector and self-annihilates into lighter mediators which subsequently decay to the Standard Model (SM) particles. Depending on the coupling strength of the mediator to the SM, the hidden…

高能物理 - 唯象学 · 物理学 2022-09-27 Kwei-Chou Yang

We consider the early universe at temperatures close to the fundamental scale of gravity (M_D << M_Planck) in models with extra dimensions. At such temperatures a small fraction of particles will experience transplanckian collisions that…

高能物理 - 理论 · 物理学 2010-01-26 Monica Borunda , Manuel Masip

The cold dark matter model successfully explains both the emergence and evolution of cosmic structures on large scales and, when we include a cosmological constant, the properties of the homogeneous and isotropic Universe. However, the cold…

宇宙学与河外天体物理 · 物理学 2020-08-04 Ivan de Martino , Sankha S. Chakrabarty , Valentina Cesare , Arianna Gallo , Luisa Ostorero , Antonaldo Diaferio

An exact parity replicates the Standard Model giving a Mirror Standard Model, SM $\leftrightarrow$ SM$'$. This "Higgs Parity" and the mirror electroweak symmetry are spontaneously broken by the mirror Higgs, $\left\langle H'\right\rangle =…

高能物理 - 唯象学 · 物理学 2020-03-18 David Dunsky , Lawrence J. Hall , Keisuke Harigaya

A variety of supergravity and string models involve hidden sectors where the hidden sectors may couple feebly with the visible sectors via a variety of portals. While the coupling of the hidden sector to the visible sector is feeble its…

高能物理 - 唯象学 · 物理学 2024-06-04 Jinzheng Li , Pran Nath

In this conference paper, we consider effective field theories of non-relativistic dark matter particles interacting with a light force mediator in the early expanding universe. We present a general framework, where to account in a…

高能物理 - 唯象学 · 物理学 2023-04-18 Simone Biondini , Nora Brambilla , Gramos Qerimi , Antonio Vairo

An analysis of sub-MeV dark photon as dark matter is given which is achieved with two hidden sectors, one of which interacts directly with the visible sector while the second has only indirect coupling with the visible sector. The formalism…

高能物理 - 唯象学 · 物理学 2021-06-30 Amin Aboubrahim , Wan-Zhe Feng , Pran Nath , Zhu-Yao Wang

Neutrino oscillations in the early Universe prior to the epoch of primordial nucleosynthesis is studied by implementing real time non-equilibrium field theory methods. We focus on two flavors of Dirac neutrinos, however, the formulation is…

高能物理 - 唯象学 · 物理学 2009-11-11 C. M. Ho , D. Boyanovsky , H. J. de Vega

We investigate the mixing of heavy gauge singlet neutrinos in a mirror matter model employing the seesaw mechanism. The parameter constraints that must be satisfied to prevent the overproduction of mirror matter in the early universe are…

高能物理 - 唯象学 · 物理学 2009-10-31 Nicole F. Bell

Recent discoveries of primordial black hole (PBH) candidates by means of high cadence microlensing open the way to a physical understanding of the formation of dark matter as a chapter in the thermal history of the Universe. Two…

宇宙学与河外天体物理 · 物理学 2025-04-17 Jeremy Mould

We explore a simple solution to the cosmological challenges of the original Mirror Twin Higgs (MTH) model that leads to interesting implications for experiment. We consider theories in which both the standard model and mirror neutrinos…

高能物理 - 唯象学 · 物理学 2017-08-02 Zackaria Chacko , Nathaniel Craig , Patrick J. Fox , Roni Harnik

We consider the thermal effects into the evaluation of the dark matter production process. With the assistance of the right handed neutrinos, the freeze-in massive particle dark matter production history can be modified by the two-step…

高能物理 - 唯象学 · 物理学 2018-12-26 Ligong Bian , Yi-Lei Tang

We consider the temperature dynamics of hypothetical primordial hot areas in the Universe. Such areas can be produced by the primordial density inhomogeneities and can survive to the modern era, in particular due to primordial black hole…

宇宙学与河外天体物理 · 物理学 2020-12-01 K. M. Belotsky , M. M. El Kasmi , S. G. Rubin

Cosmological measurements of the radiation density in the early universe can be used as a sensitive probe of physics beyond the standard model. Observations of primordial light element abundances have long been used to place non-trivial…

宇宙学与河外天体物理 · 物理学 2016-05-19 Joel Meyers

We study the scenario of higgsino dark matter in the context of a non-standard cosmology with a period of matter-domination prior to Big-Bang nucleosynthesis. Matter-domination changes the dark matter relic abundance if it ends via…

高能物理 - 唯象学 · 物理学 2016-11-03 Luis Aparicio , Michele Cicoli , Bhaskar Dutta , Francesco Muia , Fernando Quevedo

It is shown, in the framework of the Thomas-Fermi model at finite temperature, that a cooling non-degenerate gas of massive neutrinos will, at a certain temperature, become unstable and undergo a first-order phase transition in which…

天体物理学 · 物理学 2007-05-23 Neven Bilic , Raoul D. Viollier