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Open AccessJournal ArticleDOI

New stellar constraints on dark photons

TLDR
In this article, the stellar production of vector states V within the minimal model of "dark photons" was studied and it was shown that when the Stuckelberg mass of the dark vector becomes smaller than plasma frequency, the emission rate is dominated by the production of the longitudinal modes of V, and scales as κ 2 m V 2, where κ and m V are the mixing angle with the photon and the mass of a dark state.
About
This article is published in Physics Letters B.The article was published on 2013-10-01 and is currently open access. It has received 294 citations till now. The article focuses on the topics: Dark photon & Dark state.

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Gravitational production of hidden photon dark matter in light of the XENON1T excess

TL;DR: In particular, the high-scale inflation is consistent with the absorption of 3 keV bosonic dark matter with kinetic mixing of the order of 10 − 15 as mentioned in this paper, and the minimally gravitational production provides a viable mechanism for obtaining a correct relic hidden photon abundance.
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Scalar direct detection: In-medium effects

TL;DR: In this paper, the authors implement the in-medium effects for scalar DM detection, using thermal field theory techniques, and show that the reach of a large class of direct DM detection experiments searching for light scalars is significantly reduced.
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New physics and the black hole mass gap

TL;DR: In this paper, the authors argue that future observations of the black hole population will allow one to test this prediction, and use it to put constraints on new particles, such as axions, that would cause an additional instability.
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EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade

R. Alves Batista, +131 more
TL;DR: The European Consortium for Astroparticle Theory (EuCAPT) white paper as mentioned in this paper explores upcoming theoretical opportunities and challenges for our field of research with particular emphasis on the possible synergies among different subfields, and the prospects for solving the most fundamental open questions with multi-messenger observations.
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Materials Informatics for Dark Matter Detection

TL;DR: In this article, light WIMPs are assumed to be weakly interacting massive particles (WIMPs) with a mass in the GeV-to-TeV range.
References
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Journal ArticleDOI

Two U(1)'s and Epsilon Charge Shifts

TL;DR: If new particles are gauged by a new U(1) then their electromagnetic charges may be shifted by a calculable amount as mentioned in this paper, which is the case in the case of the current article.
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A theory of dark matter

TL;DR: In this paper, the authors proposed a light boson invoked by XDM to mediate a large inelastic scattering cross section for the DAMA annual modulation signal at low velocities at redshift, which could produce observable effects on the ionization history of the universe.
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Secluded WIMP Dark Matter

TL;DR: In this article, a generic mechanism via which thermal relic WIMP dark matter may be decoupled from the Standard Model, namely through a combination of WIMPs annihilation to metastable mediators with subsequent delayed decay to Standard Model states, is considered.
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The Low-Energy Frontier of Particle Physics

TL;DR: Most embeddings of the Standard Model into a more unified theory, in particular those based on supergravity or superstrings, predict the existence of a hidden sector of particles that have only very weak interactions with visible-sector Standard Model particles.
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WISPy cold dark matter

TL;DR: Very weakly interacting slim particles (WISPs) such as axion-like particles (ALPs) or hidden photons (HPs), may be non-thermally produced via the misalignment mechanism in the early universe and survive as a cold dark matter population until today as mentioned in this paper.
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