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相关论文: The Irreducible Axion Background

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We investigate the possible parametric growth of photon amplitudes in a background of axion-like particle (ALP) dark matter. The observed extragalactic background radiation limits the allowed enhancement effect. We derive the resulting…

宇宙学与河外天体物理 · 物理学 2019-07-11 Günter Sigl , Pranjal Trivedi

Dark matter particles could be superheavy (mass $M_X\gtrsim10^9~$GeV) provided that their lifetime $\tau_X$ is extremely long, i.e. greater than $\simeq 10^{22}~$yr. Such stringent constraints on $\tau_X$ are generally obtained by limiting…

高能物理 - 唯象学 · 物理学 2025-09-16 O. Deligny

The dark photon is a well motivated candidate for the dark matter which comprises most of the mass of our visible Universe, leading to worldwide experimental and observational efforts towards its discovery. A primary tool in this search is…

高能物理 - 实验 · 物理学 2026-04-01 Yuan-Hann Chang , Cheng-Wei Chiang , Hien Thi Doan , Nick Houston , Jinmian Li , Tianjun Li , Lina Wu , Xin Zhang

Axion particles can form macroscopic condensates, whose size can be galactic in scale for models with very small axion masses $m\sim10^{-22}$ eV, and which are sometimes referred to under the name of Fuzzy Dark Matter. Many analyses of…

高能物理 - 唯象学 · 物理学 2018-02-21 Joshua Eby , Michael Ma , Peter Suranyi , L. C. R. Wijewardhana

Dark photons that are sufficiently light and/or weakly-interacting represent a compelling vision of dark matter. Dark photon decay into three photons, which we call the dark photon trident, can be the dominant channel when the dark photon…

高能物理 - 唯象学 · 物理学 2025-07-22 Tim Linden , Thong T. Q. Nguyen , Tim M. P. Tait

It is usually assumed that dark matter is produced during the radiation dominated era. There is, however, no direct evidence for radiation domination prior to big-bang nucleosynthesis. Two non-standard thermal histories are considered. In…

天体物理学 · 物理学 2008-11-26 Daniel Grin , Tristan L. Smith , Marc Kamionkowski

Axions that couple to electromagnetism are produced in the early Universe by, among other channels, freeze-in via the Primakoff process. For sufficiently large axion masses, the same coupling causes the axions to decay into two photons,…

高能物理 - 唯象学 · 物理学 2025-10-24 Ziwen Yin , Hanyu Cheng , Eleonora Di Valentino , Naomi Gendler , David J. E. Marsh , Luca Visinelli

Axions and dark photons are common in many extensions of the Standard Model. The dark axion portal -- an axion coupling to the dark photon and photon -- can significantly modify their phenomenology. We study the cosmological constraints on…

高能物理 - 唯象学 · 物理学 2024-04-01 Heejoung Hong , Ui Min , Minho Son , Tevong You

We revisit constraints on dark photons with masses below ~ 100 MeV from the observations of Supernova 1987A. If dark photons are produced in sufficient quantity, they reduce the amount of energy emitted in the form of neutrinos, in conflict…

高能物理 - 唯象学 · 物理学 2019-06-04 Jae Hyeok Chang , Rouven Essig , Samuel D. McDermott

If a component of cosmological dark matter is made up of massive particles - such as sterile neutrinos - that decay with cosmological lifetime to emit photons, the reionization history of the universe would be affected, and cosmic microwave…

宇宙学与河外天体物理 · 物理学 2015-06-05 S. Yeung , M. H. Chan , M. -C. Chu

We study inelastic dark matter produced via freeze-in through a light mediator with a mass splitting below the electron-positron threshold. In this regime, the heavier dark matter state is naturally long-lived compared to the age of the…

高能物理 - 唯象学 · 物理学 2025-09-25 Gordan Krnjaic , David McKeen , Riku Mizuta , Gopolang Mohlabeng , David E. Morrissey , Douglas Tuckler

Sub-GeV dark matter particles can annihilate or decay producing e^\pm pairs which upscatter the low-energy photon fields in the Galaxy and generate an X-ray emission (via the Inverse Compton effect). Using X-ray data from XMM-Newton,…

高能物理 - 唯象学 · 物理学 2025-07-18 Marco Cirelli , Nicolao Fornengo , Jordan Koechler , Elena Pinetti , Brandon M. Roach

Bounds are derived on the axion-like particle (ALP) to two-photon coupling in the mass range $2.65-5.27$ eV. The bounds are obtained by searching for the signal from ALP decay in the Multi Unit Spectroscopic Explorer (MUSE) observations of…

宇宙学与河外天体物理 · 物理学 2023-10-04 Elisa Todarello

From considering the effect of gamma-gamma interactions on recently observed TeV gamma-ray spectra, improved limits are set to the density of extragalactic infrared (IR) photons which are robust and essentially model-independent. The…

It is possible that the strongest interactions between dark matter and the Standard Model occur via the neutrino sector. Unlike gamma rays and charged particles, neutrinos provide a unique avenue to probe for astrophysical sources of dark…

Existing searches for cosmic axions relics have relied heavily on the axion being non-relativistic and making up dark matter. However, light axions can be copiously produced in the early Universe and remain relativistic today, thereby…

高能物理 - 唯象学 · 物理学 2022-11-10 Jeff A. Dror , Hitoshi Murayama , Nicholas L. Rodd

Recently it has been pointed out that a cosmic background of relativistic axion-like particles (ALPs) would be produced by the primordial decays of heavy fields in the post-inflation epoch, contributing to the extra-radiation content in the…

宇宙学与河外天体物理 · 物理学 2016-05-25 Carmelo Evoli , Matteo Leo , Alessandro Mirizzi , Daniele Montanino

We show that a stable vortex soliton, carrying a constant magnetic flux, exists in the homogeneous medium of axions with a constant time-derivative. Axions can be bound in the vortex, having energy less than the axion mass. If the observed…

高能物理 - 唯象学 · 物理学 2024-04-02 Deog Ki Hong , Stephen J. Lonsdale

The axion, which has yet to be discovered, is a promising candidate for dark matter that emerges from Peccei-Quinn theory. This article presents the search for axion dark matter with the "Student Project for an Axion Cavity Experiment"…

高能物理 - 实验 · 物理学 2025-10-29 M. A. Akgümüs , N. Salama , J. Egge , E. Garutti , M. Maroudas , L. H. Nguyen , D. Leppla-Weber

Dark matter particles need not be completely stable, and in fact they may be decaying now. We consider this possibility in the frameworks of universal extra dimensions and supersymmetry with very late decays of WIMPs to Kaluza-Klein…

天体物理学 · 物理学 2009-06-23 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari