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相关论文: New bounds on millicharged particles from cosmolog…

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A variety of beyond the standard model scenarios contain very light hidden sector U(1) gauge bosons undergoing kinetic mixing with the photon. The resulting oscillation between ordinary and hidden photons leads to spectral distortions of…

宇宙学与河外天体物理 · 物理学 2015-12-16 Kerstin E. Kunze , Miguel A. Vazquez-Mozo

It is argued that if extragalactic magnetic fields are smaller than 2x10^{-12} G the flux of ultra-high energy photons of (a few)x10^{-1} eV cm^{-2}s^{-1}sr^{-1} predicted in the top-down models of UHE CR implies similar flux of the diffuse…

天体物理学 · 物理学 2007-05-23 P. G. Tinyakov

We explore the cosmological consequences of kinetically mixed dark photons with a mass between 1 MeV and 10 GeV, and an effective electromagnetic fine structure constant as small as $10^{-38}$. We calculate the freeze-in abundance of these…

高能物理 - 唯象学 · 物理学 2014-09-05 Anthony Fradette , Maxim Pospelov , Josef Pradler , Adam Ritz

Recent measurements of cosmic ray electron energy spectra suggest that above 10 GeV there may be deviations from a single power law spectrum. There are hints (ATIC) for a bump occurring between 100 GeV and 1TeV, meaning that there might be…

高能天体物理现象 · 物理学 2017-08-23 Andrea Tartari , Massimo Gervasi , Giorgio Sironi , Mario Zannoni , Sebastiano Spinelli

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

We present an upper limit on the polarization of the Cosmic Microwave Background at 7 degree angular scales in the frequency band between 26 and 36 GHz, produced by the POLAR experiment. The campaign produced a map of linear polarization…

Various extensions of the Standard Model predict the existence of hidden photons kinetically mixing with the ordinary photon. This mixing leads to oscillations between photons and hidden photons, analogous to the observed oscillations…

高能物理 - 唯象学 · 物理学 2009-03-30 Alessandro Mirizzi , Javier Redondo , Guenter Sigl

Charged particles in an Abelian Coulomb phase are non-local infraparticles that are surrounded by a cloud of soft photons which extends to infinity. Gauss' law prevents the existence of charged particles in a periodic volume. In a…

高能物理 - 格点 · 物理学 2022-11-28 G. Kanwar , A. Mariani , J. C. Pinto Barros , U. J. Wiese

Circularly polarized colliding laser pulses can create abundant electron-positron pair plasma [A. R. Bell and J. G. Kirk, Phys. Rev. Lett. 101, 200403 (2008)], which scattering the incoming electromagnetic waves can prevent them from…

The relic abundance of light millicharged particles (MCPs) with the electric charge $e' = 5\cdot 10^{-5} e$ and with the mass slightly below or above the electron mass is calculated. The abundance depends on the mass ratio $\eta=m_X/m_e$…

高能物理 - 唯象学 · 物理学 2017-05-18 A. D. Dolgov , A. S. Rudenko

The V-mode polarization of the Cosmic Microwave Background is discussed in a weakly magnetized plasma. The VV and VT angular power spectra are computed for adiabatic initial conditions of the Einstein-Boltzmann hierarchy. Depending upon the…

宇宙学与河外天体物理 · 物理学 2015-05-14 Massimo Giovannini

The pseudoscalar-photon mixing in presence of large scale magnetic field induces polarization in light from distant cosmological sources. We study the effect of these pseudoscalars or axion like particles (ALPs) on Cosmic Microwave…

高能物理 - 唯象学 · 物理学 2013-01-04 Prabhakar Tiwari

We propose a new experiment at the Large Hadron Collider (LHC) that offers a powerful and model-independent probe for milli-charged particles. This experiment could be sensitive to charges in the range $10^{-3}e - 10^{-1}e$ for masses in…

高能物理 - 唯象学 · 物理学 2015-07-01 Andrew Haas , Christopher S. Hill , Eder Izaguirre , Itay Yavin

Heat transfer between baryons and millicharged dark matter has been invoked as a possible explanation for the anomalous 21-cm absorption signal seen by EDGES. Prior work has shown that the solution requires that millicharged particles make…

宇宙学与河外天体物理 · 物理学 2019-07-24 Cyril Creque-Sarbinowski , Lingyuan Ji , Ely D. Kovetz , Marc Kamionkowski

We constrain the coupling of thermally-produced axion-like particles (here axions) with photons and gluons, using data from the cosmic microwave background (CMB) spectra and baryon acoustic oscillations. The axion possesses an explicit soft…

宇宙学与河外天体物理 · 物理学 2022-09-12 Luca Caloni , Martina Gerbino , Massimiliano Lattanzi , Luca Visinelli

The observation of a non-vanishing rotation of linear polarized laser light after passage through a strong magnetic field by the PVLAS collaboration has renewed the interest in light particles coupled to photons. Axions are a species of…

高能物理 - 唯象学 · 物理学 2008-11-26 Joerg Jaeckel

Axion-like particles are hypothetical new light (sub-eV) bosons predicted in some extensions of the Standard Model of particle physics. In astrophysical environments comprising high-energy gamma rays and turbulent magnetic fields, the…

高能天体物理现象 · 物理学 2019-08-14 Pierre Brun , Denis Wouters

After a brief review of different types of scenarios suggested for the solution of the problem of galactic and intergalactic magnetic field generation, the mechanism based on the electric current induction by hypothetical millicharged…

宇宙学与河外天体物理 · 物理学 2015-09-02 A. D. Dolgov

In these proceedings we use recent LHC heavy-ion data to set a limit on axion-like particles coupling to electromagnetism with mass in the range 10-100 GeV. We recast ATLAS data as per the strategy proposed in 1607.06083, and find results…

高能物理 - 唯象学 · 物理学 2017-09-22 Simon Knapen , Tongyan Lin , Hou Keong Lou , Tom Melia

The observed interaction energy of cosmic rays with atmospheric nuclei reaches up to a PeV in the center of mass. We compute nucleon-nucleon and nucleon-neutrino cross sections for various generic parton cross sections appearing in string…

高能物理 - 唯象学 · 物理学 2007-05-23 Guenter Sigl