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相关论文: Cosmic Millicharge Background and Reheating Probes

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Observers have demonstrated that it is now feasible to measure the cosmic microwave background (CMB) temperature at high redshifts. We explore the possible constraints on cosmology which might ultimately be derived from such measurements.…

天体物理学 · 物理学 2009-11-07 John M. LoSecco , Grant J. Mathews , Yun Wang

Understanding the properties of dark matter has proved to be one of the most challenging problems of particle phenomenology. In this paper, we have tried to understand the phenomenology of dark matter in light of very well understood…

高能物理 - 唯象学 · 物理学 2018-11-28 Debaprasad Maity , Pankaj Saha

We study slow roll single field inflationary scenario and the production of non-thermal fermionic dark matter, together with standard model Higgs, during reheating. For the inflationary scenario, we have considered two models of polynomial…

宇宙学与河外天体物理 · 物理学 2022-11-29 Anish Ghoshal , Gaetano Lambiase , Supratik Pal , Arnab Paul , Shiladitya Porey

The existence of millicharged dark matter (mDM) can leave a measurable imprint on 21-cm cosmology through mDM-baryon scattering. However, the minimal scenario is severely constrained by existing cosmological bounds on both the fraction of…

高能物理 - 唯象学 · 物理学 2019-12-25 Hongwan Liu , Nadav Joseph Outmezguine , Diego Redigolo , Tomer Volansky

The large-angular-scale falloff in the autocorrelation function for the cosmic microwave background (CMB) temperature has long intrigued cosmologists and fueled speculation about suppressed superhorizon power. Here we highlight an…

宇宙学与河外天体物理 · 物理学 2023-11-13 Jahmour J. Givans , Marc Kamionkowski

Forthcoming cosmic microwave background experiments (CMB) will provide precise new tests of structure-formation theories. The geometry of the Universe may be determined robustly, and the classical cosmological parameters, such as the…

天体物理学 · 物理学 2007-05-23 Marc Kamionkowski

The simplest cosmologies motivate the consideration of dark matter subcomponents that interact significantly with normal matter. Moreover, such strongly-coupled relics may have evaded detection to date if upon encountering the Earth they…

高能物理 - 唯象学 · 物理学 2023-02-15 Asher Berlin , Hongwan Liu , Maxim Pospelov , Harikrishnan Ramani

This work presents a detailed analysis of Cosmic Microwave Background (CMB) radiation intensity observations. The CMB is a relic of the Big Bang and its study greatly enhances our knowledge of cosmology. This work has led to new values for…

天体物理学 · 物理学 2007-05-23 Henrik P. Nordberg , George F. Smoot

We compute the thermalization of a hidden sector consisting of minicharged fermions (MCPs) and massless hidden photons in the early Universe. The precise measurement of the anisotropies of the cosmic microwave background (CMB) by Planck and…

高能物理 - 唯象学 · 物理学 2014-03-11 Hendrik Vogel , Javier Redondo

We propose a novel idea to discover millicharged particles (mCPs) captured by the earth during its existence. It has been demonstrated that the mCPs accumulation inside the earth leads to the enhancement of its number density much larger…

高能物理 - 唯象学 · 物理学 2025-06-06 Chrisna Setyo Nugroho

We update dark radiation constraints on millicharged particle (MCP) and gauged baryon-number-minus-lepton-number ($B-L$) extensions of the Standard Model (SM). In these models, a massive SM gauge singlet mediator couples the SM plasma to…

高能物理 - 唯象学 · 物理学 2023-05-25 Peter Adshead , Pranjal Ralegankar , Jessie Shelton

The Cosmic Microwave Background (CMB) is a relict of the early universe. Its perfect 2.725K blackbody spectrum demonstrates that the universe underwent a hot, ionized early phase; its anisotropy (about 80 \mu K rms) provides strong evidence…

天体物理仪器与方法 · 物理学 2015-06-11 Paolo de Bernardis , Silvia Masi

We intend to show how fundamental science is drawn from the patterns in the temperature and polarization fields of the cosmic microwave background (CMB) radiation, and thus to motivate the field of CMB research. We discuss the field's…

天体物理学 · 物理学 2008-11-26 Dorothea Samtleben , Suzanne Staggs , Bruce Winstein

Light dark matter is a compelling experimental target in light of stringent constraints on heavier WIMPs. However, for a sub-MeV WIMP, the universe is sufficiently well understood at temperatures below 10 MeV that there is no room for it to…

高能物理 - 唯象学 · 物理学 2018-03-02 Daniel Green , Surjeet Rajendran

The Cosmic Microwave Background Radiation (CMB) is an invaluable probe of the conditions of the early universe. Recent measurements of its spatial anisotropy have allowed accurate determinations of several fundamental cosmological…

天体物理学 · 物理学 2009-09-29 Christopher O'Dell

Spatially fluctuating primordial magnetic fields (PMFs) inhomogeneously reheat the Universe when they dissipate deep inside the horizon before recombination. Such an energy injection turns into an additional photon temperature perturbation.…

宇宙学与河外天体物理 · 物理学 2019-11-28 Shohei Saga , Atsuhisa Ota , Hiroyuki Tashiro , Shuichiro Yokoyama

If dark matter particles have an electric charge, as in models of millicharged dark matter, such particles should be accelerated in the same astrophysical accelerators that produce ordinary cosmic rays, and their spectra should have a…

高能物理 - 唯象学 · 物理学 2017-03-02 Ping-Kai Hu , Alexander Kusenko , Volodymyr Takhistov

The Cosmic Microwave Background (CMB) provides a precious window on fundamental physics at very high energy scales, possibly including quantum gravity, GUTs and supersymmetry. The CMB has already enabled defect-based rivals to inflation to…

天体物理学 · 物理学 2009-09-11 John Ellis

We consider the CMB constraints on reheating and dark matter parameter space for a specific plateau type inflationary model. The plateau inflationary models which are currently most favored models from data can be well approximated by a…

高能物理 - 唯象学 · 物理学 2019-06-07 Debaprasad Maity , Pankaj Saha

Much recent work on the cosmic microwave background (CMB) has focussed on the angular power spectrum of temperature anisotropies and particularly on the recovery of cosmological parameters from acoustic peaks in the power spectrum. However,…

天体物理学 · 物理学 2007-05-23 Marc Kamionkowski