Results 21 to 30 of about 4,135 (229)

Direct search for dark matter axions excluding ALP cogenesis in the 63- to 67-μeV range with the ORGAN experiment. [PDF]

open access: yesSci Adv, 2022
The standard model axion seesaw Higgs portal inflation (SMASH) model is a well-motivated, self-contained description of particle physics that predicts axion dark matter particles to exist within the mass range of 50 to 200 micro–electron volts.
Quiskamp A   +5 more
europepmc   +5 more sources

Predictions for axion couplings from ALP cogenesis [PDF]

open access: yesJournal of High Energy Physics, 2021
Abstract Adding an axion-like particle (ALP) to the Standard Model, with a field velocity in the early universe, simultaneously explains the observed baryon and dark matter densities. This requires one or more couplings between the ALP and photons, nucleons, and/or electrons that are predicted as functions of the ALP mass.
Raymond T. Co   +3 more
openaire   +7 more sources

Getting the most on supernova axions [PDF]

open access: yesPhysical Review D, 2023
Axion-like particles (ALPs) coupled to nucleons might be copiously emitted from a supernova (SN) core. We extend existing bounds on free-streaming ALPs to the case in which these are so strongly-interacting with the nuclear matter to be trapped in the SN
A. Lella   +6 more
semanticscholar   +1 more source

Constraining postinflationary axions with pulsar timing arrays [PDF]

open access: yesPhysical Review D, 2023
Models that produce Axion-Like-Particles (ALP) after cosmological inflation due to spontaneous $U(1)$ symmetry breaking also produce cosmic string networks.
G. Servant, P. Simakachorn
semanticscholar   +1 more source

Production and Detection of Axion-Like Particles in a HERA Dipole Magnet - Letter-of-Intent for the ALPS experiment -

open access: green, 2007
Recently, the PVLAS collaboration has reported evidence for an anomalous rotation of the polarization of light in vacuum in the presence of a transverse magnetic field. This may be explained through the production of a new light spin-zero (axion-like) neutral particle coupled to two photons.
Klaus Ehret   +7 more
openalex   +5 more sources

Extreme axions unveiled: A novel fluid approach for cosmological modeling [PDF]

open access: yesPhysical Review D, 2023
Axion-like particles (ALPs) are a well-motivated dark matter candidate that solve some of the problems in the clustering of large scale structure in cosmology.
H. Winch   +4 more
semanticscholar   +1 more source

Higher-Order Corrections to the Effective Field Theory of Low-Energy Axions [PDF]

open access: yesSymmetry, 2023
Dark matter (DM) can be composed of a collection of axions, or axion-like particles (ALPs), whose existence is due to the spontaneous breaking of the Peccei–Quinn U(1) symmetry, which is the most compelling solution of the strong CP-problem of quantum ...
Bryan Cordero-Patino   +2 more
semanticscholar   +1 more source

Hilbert series for ALP EFTs

open access: yesJournal of High Energy Physics, 2023
Axions and axion-like particles (ALPs) are ubiquitous in popular attempts to solve supercalifragilisticexpialidocious puzzles of Nature. A widespread and vivid experimental programme spanning a vast range of mass scales and decades of couplings strives ...
Christophe Grojean   +2 more
doaj   +1 more source

New bounds on axion-like particles from MicroBooNE

open access: yesJournal of High Energy Physics, 2022
Neutrino experiments lie at the edge of the intensity frontier and therefore can be exploited to search for new light particles weakly coupled to the visible sector.
Pilar Coloma   +2 more
doaj   +1 more source

A First Application of Machine and Deep Learning for Background Rejection in the ALPS II TES Detector [PDF]

open access: yesAnnals of Physics, 2023
Axions and axion‐like particles are hypothetical particles predicted in extensions of the standard model and are promising cold dark matter candidates. The Any Light Particle Search (ALPS II) experiment is a light‐shining‐through‐the‐wall experiment that
M. Meyer   +8 more
semanticscholar   +1 more source

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