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相关论文: Freeze-in Dark Matter Perturbations are Adiabatic

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We consider generic freeze-in processes for generation of Dark Matter, together with the consequent re-thermalization of the Standard Model fluid. We find that Dark Matter inherits the Standard Model adiabatic inhomogeneities on the…

高能物理 - 唯象学 · 物理学 2024-01-19 Alessandro Strumia

Dark matter freeze-in is a compelling cosmological production mechanism in which all or some of the observed abundance of dark matter is generated through feeble interactions it has with the Standard Model. In this work we present the first…

宇宙学与河外天体物理 · 物理学 2024-11-18 Nicola Bellomo , Kim V. Berghaus , Kimberly K. Boddy

Isocurvature fluctuations, where the relative number density of particle species spatially varies, can be generated from initially adiabatic, or curvature, fluctuations if the various species fall out of or were never in thermal…

宇宙学与河外天体物理 · 物理学 2024-03-20 Ian Holst , Wayne Hu , Leah Jenks

The adiabatic perturbation of dark matter is damped during the kinetic decoupling due to the collision with relativistic component on sub-horizon scales. However the isocurvature part is free from damping and could be large enough to make a…

宇宙学与河外天体物理 · 物理学 2015-11-25 Ki-Young Choi , Jinn-Ouk Gong , Chang Sub Shin

We formulate a new class of primordial perturbations called $\textit{kinetic isocurvature perturbations}$, where the mass density of dark matter is constant relative to the photon number density while the kinetic energy of dark matter…

高能物理 - 唯象学 · 物理学 2026-03-25 Kyu Jung Bae , Dhong Yeon Cheong , Jinn-Ouk Gong , Keisuke Harigaya , Chang Sub Shin

We revisit the generation of dark matter isocurvature perturbations in the curvaton model in greater detail, both analytically and numerically. As concrete examples, we investigate the cases of thermally decoupled dark matter and axionic…

宇宙学与河外天体物理 · 物理学 2018-01-10 Naoya Kitajima , David Langlois , Tomo Takahashi , Shuichiro Yokoyama

We consider a process to create quasi long-range quantum discord between the non-interacting end spins of a quantum spin chain, with the end spins weakly coupled to the bulk of the chain. The process is not only capable of creating…

量子物理 · 物理学 2018-05-21 Himadri Shekhar Dhar , Debraj Rakshit , Aditi Sen De , Ujjwal Sen

This is a review of the Cold Dark Matter model of structure formation, and its variants. The approach is largely from first principles, the main aim being to impart a basic understanding of the relevant theory with an eye to the likely…

天体物理学 · 物理学 2010-11-30 Andrew R Liddle , David H Lyth

We consider theories with a nontrivial coupling between the matter and dark energy sectors. We describe a small scale instability that can occur in such models when the coupling is strong compared to gravity, generalizing and correcting…

天体物理学 · 物理学 2009-06-23 Rachel Bean , Eanna E. Flanagan , Mark Trodden

We study the importance of a frozen-in dark matter production regime, where the dark matter particle is produced via kinematically forbidden decays that arise from significant thermal correction to the mass a mediator particle in the…

高能物理 - 唯象学 · 物理学 2020-03-31 Luc Darmé , Andrzej Hryczuk , Dimitrios Karamitros , Leszek Roszkowski

Determining the equation of state of dark energy with astronomical observations is crucially important to understand the nature of dark energy. In performing a likelihood analysis of the data, especially of the cosmic microwave background…

宇宙学与河外天体物理 · 物理学 2011-07-21 Jie Liu , Mingzhe Li , Xinmin Zhang

The primordial fluctuations on large scales are adiabatic, but on smaller scales this need not be the case. Here we derive the general analytical framework to compute the stochastic gravitational wave background induced by primordial cold…

宇宙学与河外天体物理 · 物理学 2022-03-22 Guillem Domènech , Samuel Passaglia , Sébastien Renaux-Petel

If dark energy interacts with dark matter, this gives a new approach to the coincidence problem. But interacting dark energy models can suffer from pathologies. We consider the case where the dark energy is modelled as a fluid with constant…

天体物理学 · 物理学 2008-11-26 Jussi Valiviita , Elisabetta Majerotto , Roy Maartens

We investigate the possibility of dark matter being a pure geometrical effect, rather than a particle or a compact object, by exploring a specific modified gravity model: mimetic dark matter. We present an alternative formulation of the…

宇宙学与河外天体物理 · 物理学 2020-08-18 Ali Rida Khalifeh , Nicola Bellomo , José Luis Bernal , Raul Jimenez

The universe has evolved through several phases as its various constituents dominated its energy content. Candidate dark matter particles may have undergone freeze-out during any such phase. While the standard freeze-out scenarios have been…

高能物理 - 唯象学 · 物理学 2021-08-18 Saleh Hamdan

We examine a scenario for freeze-in production of dark matter, which occurs due to the large thermal correction to the mass of a decaying mediator particle present in the thermal bath of the early Universe. We show that the decays, which…

高能物理 - 唯象学 · 物理学 2022-03-14 Partha Konar , Rishav Roshan , Sudipta Show

The mimetic gravity theory is one of the interesting modified gravity theories, which aims to unify the matter component of our universe within the power of gravity. The mimetic-like theory can also be responsible for primordial…

广义相对论与量子宇宙学 · 物理学 2024-05-14 Anxianyi Xiong , Xin-zhe Zhang , Taotao Qiu

We point out an earlier implementation of the "freeze-in" mechanism for the production of very weakly-interacting dark matter. We also clarify a footnote given in 0911.1120 regarding this eariler paper.

高能物理 - 唯象学 · 物理学 2011-12-08 John McDonald

We study a novel dark matter production mechanism based on the freeze-in through semi-production, i.e. the inverse semi-annihilation processes. A peculiar feature of this scenario is that the production rate is suppressed by a small initial…

高能物理 - 唯象学 · 物理学 2021-06-08 Andrzej Hryczuk , Maxim Laletin

Fluctuations in the mass and decay rate of a heavy particle which for some period dominates the energy density of the universe are known to lead to adiabatic density perturbations. We show that generically the annihilation cross section of…

天体物理学 · 物理学 2009-11-10 Christian W. Bauer , Michael L. Graesser , Michael P. Salem
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