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M87 hosts a 3-6 billion solar mass black hole with a remarkable relativistic jet that has been regularly monitored in radio to TeV bands. However, hard X-ray emission \gtrsim 10keV, which would be expected to primarily come from the jet or…

高能天体物理现象 · 物理学 2017-11-07 Ka-Wah Wong , Rodrigo S. Nemmen , Jimmy A. Irwin , Dacheng Lin

We measure the ionizing photon production efficiency ($\xi_{ion}$) of low-mass galaxies ($10^{7.8}$-$10^{9.8}$ $M_{\odot}$) at $1.4<z<2.7$, allowing us to better understand the contribution of dwarf galaxies to the ionizing background and…

The mixing of photons with axion-like particles (ALPs) in the large-scale magnetic field $B$ changes the polarization angle of a linearly polarized photon beam from active galactic nuclei in radio galaxies as it propagates over cosmological…

高能天体物理现象 · 物理学 2012-06-13 D. Horns , L. Maccione , A. Mirizzi , M. Roncadelli

Decaying axion-like particles (ALP) with masses in the eV range which might occupy dark matter halos of the Milky Way and other galaxies produce a characteristic "bump" feature in the spectrum of extragalactic background light (EBL). This…

高能物理 - 唯象学 · 物理学 2020-04-20 A. Korochkin , A. Neronov , D. Semikoz

Ultralight axion-like particles can contribute to the dark matter near the Sun, leading to a distinct, stochastic signature in terrestrial experiments. We search for such particles through their neutron-spin coupling by re-analyzing…

高能物理 - 唯象学 · 物理学 2023-04-05 Junyi Lee , Mariangela Lisanti , William A. Terrano , Michael Romalis

Ultra light particles $(m_a \sim 10^{-21}eV-10^{-22}eV)$ with axion-like couplings to other particles can be candidates for fuzzy dark matter (FDM) if the axion decay constant $f_a\sim 10^{17}GeV$. If a compact star is immersed in such a…

高能物理 - 唯象学 · 物理学 2020-04-15 Tanmay Kumar Poddar , Subhendra Mohanty , Soumya Jana

Axion-like particles (ALPs) are hypothetical pseudoscalar bosons, natural in extensions of the Standard Model. Their interactions with ordinary matter and radiation are suppressed, making it challenging to detect them in laboratory…

高能物理 - 唯象学 · 物理学 2025-03-27 S. V. Troitsky

We study MeV-scale electrophilic Feebly Interacting Particles (FIPs), that may be abundantly produced in Supernova (SN) explosions, escape the star and decay into electrons and positrons. This exotic injection of leptons in the Milky Way…

高能物理 - 唯象学 · 物理学 2024-05-29 Pedro De la Torre Luque , Shyam Balaji , Pierluca Carenza

Hidden sector particles with sub-GeV masses like hidden U(1) gauge bosons, the NMSSM CP-odd Higgs, and other axion-like particles are experimentally little constrained as they interact only very weakly with the visible sector. For masses…

高能物理 - 唯象学 · 物理学 2010-08-27 Sarah Andreas , Andreas Ringwald

We show that the measured abundance of ultra-faint lensed galaxies at $z\approx 6$ in the Hubble Frontier Fields (HFF) provides stringent constraints on the parameter space of i) Dark Matter models based on keV sterile neutrinos; ii) the…

宇宙学与河外天体物理 · 物理学 2017-02-15 Nicola Menci , Alexander Merle , Maximilian Totzauer , Aurel Schneider , Andrea Grazian , Marco Castellano , Norma G. Sanchez

Compact, low-mass galaxies with strong nebular emission are considered promising candidates for efficient ionizing photon production and escape. We present a spatially resolved analysis of 189 galaxies at redshifts $z \sim 6.7-7.6$ in JADES…

星系天体物理 · 物理学 2025-07-23 Cheqiu Lyu , Enci Wang , Junxian Wang , Cheng Jia , Jie Song , Yangyao Chen , Zeyu Chen , Haoran Yu , Chengyu Ma , Jinyang Wang , Yifan Wang , Xu Kong

We propose a microwave-laser-mixed three-beam stimulated resonant photon collider, which enables access to axion-like particles in the meV mass range. Collisions between a focused pulse laser beam and a focused microwave pulse beam directly…

高能物理 - 唯象学 · 物理学 2024-07-02 Kensuke Homma , Yuri Kirita , Takafumi Miyamaru , Takumi Hasada , Airi Kodama

Axion stars could form binaries with neutron stars. Given the extremely strong external magnetic field exhibited by individual neutron stars, there can be a substantial conversion of axions to photons in these binaries. The photon emission…

高能天体物理现象 · 物理学 2022-02-23 Chris Kouvaris , Tao Liu , Kun-Feng Lyu

If axions exist they are efficiently produced in the hot and dense interior of stars, providing a novel energy-loss mechanism. In order to avoid a conflict with the observed properties of stars, one can derive a lower limit on the…

高能物理 - 唯象学 · 物理学 2008-02-03 Georg Raffelt

Axion-like particles (ALPs) and photons inter-convert in the presence of a magnetic field. At keV energies in the environment of galaxy clusters, the conversion probability can become unsuppressed for light ALPs. Conversion of thermal X-ray…

高能物理 - 唯象学 · 物理学 2016-07-06 Joseph P. Conlon , M. C. David Marsh , Andrew J. Powell

Axion-like particles with masses in the keV-GeV range have a profound impact on the cosmological evolution of our Universe, in particular on the abundance of light elements produced during Big Bang Nucleosynthesis. The resulting limits are…

高能物理 - 唯象学 · 物理学 2020-06-09 Paul Frederik Depta , Marco Hufnagel , Kai Schmidt-Hoberg

We report significant hard X-ray excesses in the energy range 2-8 keV for two nearby isolated neutron stars RX J1856.6-3754 and RX J0420.0-5022. These neutron stars have previously been observed in soft X-rays to have nearly thermal spectra…

高能天体物理现象 · 物理学 2020-11-23 Christopher Dessert , Joshua W. Foster , Benjamin R. Safdi

We report preliminary results from an arcsecond-resolution X-ray survey of nearby galaxies using ACIS on board Chandra. The total sample consists of 41 low-luminosity AGNs, including Seyferts, LINERs, and LINER/H II transition objects. In…