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In the inhomogeneous Universe, the cosmological conversion of dark photons into ordinary photons (and vice versa) may happen at a great number of resonance redshifts. This alters the CMB observed energy spectrum and degree of small-scale…

宇宙学与河外天体物理 · 物理学 2020-04-15 Kyrylo Bondarenko , Josef Pradler , Anastasia Sokolenko

A dark photon may kinetically mix with the Standard Model photon, leading to observable cosmological signatures. The mixing is resonantly enhanced when the dark photon mass matches the primordial plasma frequency, which depends sensitively…

宇宙学与河外天体物理 · 物理学 2020-12-11 Andrea Caputo , Hongwan Liu , Siddharth Mishra-Sharma , Joshua T. Ruderman

Dark photon dark matter will resonantly convert into visible photons when the dark photon mass is equal to the plasma frequency of the ambient medium. In cosmological contexts, this transition leads to an extremely efficient, albeit…

宇宙学与河外天体物理 · 物理学 2020-07-15 Samuel J. Witte , Salvador Rosauro-Alcaraz , Samuel D. McDermott , Vivian Poulin

Electromagnetic field in nuclear matter and nuclei are studied. In the nuclear matter, because the expectation value of the electric charge density operator is not zero, different in vacuum, the U(1) local gauge symmetry of electric charge…

核理论 · 物理学 2009-11-07 Bao-Xi Sun , Xiao-Fu Lu , Peng-Nian Shen , En-Guang Zhao

A dark photon may kinetically mix with the ordinary photon, inducing oscillations with observable imprints on cosmology. Oscillations are resonantly enhanced if the dark photon mass equals the ordinary photon plasma mass, which tracks the…

宇宙学与河外天体物理 · 物理学 2020-12-11 Andrea Caputo , Hongwan Liu , Siddharth Mishra-Sharma , Joshua T. Ruderman

We show that the effective gauge field for photons provides a versatile platform for controlling the flow of light. As an example we consider a photonic resonator lattice where the coupling strength between nearest neighbor resonators are…

光学 · 物理学 2015-06-17 Kejie Fang , Shanhui Fan

Light dark photons are subject to various plasma effects, such as Debye screening and resonant oscillations, which can lead to a more complex cosmological evolution than is experienced by conventional cold dark matter candidates.…

高能物理 - 唯象学 · 物理学 2020-04-01 Samuel D. McDermott , Samuel J. Witte

Using a multiple-lens plane algorithm, we study light propagation in inhomogeneous universes, for 43 different COBE-normalized Cold Dark Matter models, with various values of the density parameter Omega_0, cosmological constant lambda_0,…

天体物理学 · 物理学 2009-11-06 Premana Premadi , Hugo Martel , Richard Matzner , Toshifume Futamase

We compute the value of effective photon mass $m_\gamma$ at one-loop level in QED in the background of small ($10^{10}\,\text{g} \lesssim M \ll 10^{16}\,\text{g}$) spherically symmetric black hole in asymptotically flat spacetime. This…

高能物理 - 理论 · 物理学 2017-04-26 Slava Emelyanov

The resonant conversion, within the inter-galactic medium, of regular photons into dark photons amplifies the anisotropy observed in the CMB, thereby imposing stringent constraints on the existence of light dark photons. In this study, we…

Dark photons, a generic class of light gauge bosons that interact with the Standard Model (SM) exclusively through kinetic mixing, arise naturally in many gauge extensions of the SM. Motivated by these theoretical considerations, we present…

高能物理 - 唯象学 · 物理学 2025-12-10 Xun-Jie Xu , Boting Zhou

Photons, as quanta of electromagnetic fields, determine the electromagnetic properties of an extremely hot and dense medium. Considering the properties of photons in the interacting medium of charged particles, we explicitly calculate the…

高能物理 - 唯象学 · 物理学 2018-01-17 Samina Masood

A hypothetical photon mass, $m_{\gamma}$, can produce a frequency-dependent vacuum dispersion of light, which leads to an additional time delay between photons with different frequencies when they propagate through a fixed distance. The…

宇宙学与河外天体物理 · 物理学 2024-04-29 Jing-Yu Ran , Bao Wang , Jun-Jie Wei

The detection of massless kinetically-mixed dark photons is notoriously difficult, as the effect of this mixing can be removed by a field redefinition in vacuum. In this work, we study the prospect of detecting massless dark photons in the…

高能物理 - 唯象学 · 物理学 2023-05-09 Asher Berlin , Jeff A. Dror , Xucheng Gan , Joshua T. Ruderman

The first objective of this thesis is to fill the lack in cosmology of a description on the past light cone: the null hypersurface on which observed signals propagate. Its second goal is to evaluate the importance of inhomogeneities in the…

宇宙学与河外天体物理 · 物理学 2013-09-26 Fabien Nugier

I consider electro-weak (EW) masses and interactions generated for photons by vacuum expectation values of Stueckelberg and Higgs fields. I provide a prescription to relate their parametric values to a cosmological range derived from a…

高能物理 - 唯象学 · 物理学 2024-04-02 Lorenzo Gallerani Resca

Light propagation in cosmology is usually studied in the geometrical optics approximation which requires the spacetime curvature to be much smaller than the light wavenumber. However, for non-fuzzy particle dark matter the curvature is…

宇宙学与河外天体物理 · 物理学 2025-09-09 Sofie Marie Koksbang , Syksy Rasanen

The dark photon is a new gauge boson that naturally arises in many beyond the Standard Model theoretical models, featuring interactions that resemble quantum electrodynamics. Due to this feature, it is often considered the portal between…

高能物理 - 唯象学 · 物理学 2026-03-03 L. Angel , G. Casse , G. Gambini , A. S. de Jesus , V. Kozhuharov , A. Machado , F. S. Queiroz , E. Segreto , J. Smirnov

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

Coincidence imaging, also known as ghost imaging, is a technique that exploits correlations between two particles to reconstruct information about a specimen. The particle that relays the spatial information about the object remains…

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