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In this work we revisit five different point sources within or behind galaxy clusters in order to constrain the coupling constant between axion-like particles (ALPs) and photons. We use three distinct machine learning (ML) techniques and…

宇宙学与河外天体物理 · 物理学 2022-06-15 Simon Schallmoser , Sven Krippendorf , Francesca Chadha-Day , Jochen Weller

Axions solve the Strong CP Problem and are a cold dark matter candidate. The combined constraints from accelerator searches, stellar evolution limits and cosmology suggest that the axion mass is in the range $3 \cdot 10^{-3} > m_a >…

高能物理 - 唯象学 · 物理学 2007-05-23 Pierre Sikivie

In collisions of galaxy clusters, the lack of displacement between dark matter and galaxies suggests that the dark matter scattering depth is small. This yields an upper limit on the dark matter cross section if the dark matter column…

宇宙学与河外天体物理 · 物理学 2025-08-25 David Wittman , Scott Adler , Rodrigo Stancioli

Dark photon dark matter that has a kinetic mixing with the Standard Model photon can resonantly convert in environments where its mass $m_{A'}$ coincides with the plasma frequency. We show that such conversion in neutron stars or accreting…

高能物理 - 唯象学 · 物理学 2023-09-14 Edward Hardy , Ningqiang Song

Galaxies accrete their mass by means of both smooth accretion from the cosmic web, and the mergers of smaller entities. We wish to quantify the respective role of these two modes of accretion, which could determine the morphological types…

宇宙学与河外天体物理 · 物理学 2017-11-15 Benjamin L'Huillier , Francoise Combes , Benoit Semelin

The mass of the axion-like particles could be constrained by the observed black hole spin distribution. In this work, we update the previous calculations using the recently improved superradiance formula, which is much more accurate. The…

广义相对论与量子宇宙学 · 物理学 2023-04-05 Lei-dong Cheng , Hong Zhang , Shou-shan Bao

Clusters of galaxies generally form by the gravitational merger of smaller clusters and groups. Major cluster mergers are the most energetic events in the Universe since the Big Bang. Some of the basic physical properties of mergers will be…

天体物理学 · 物理学 2015-06-24 Craig L. Sarazin

Mixing between ultralight bosons and the Standard Model photon may allow access to the hitherto invisible Universe. In the presence of plasma, photons are dressed with an effective mass which will influence the conversion between the two.…

高能物理 - 唯象学 · 物理学 2024-10-01 Enrico Cannizzaro , Thomas F. M. Spieksma

Dark matter (DM) is a new type of invisible matter introduced to explain various features of recent astrophysical observations, including galaxy rotation curves and other fundamental characteristics of our universe. DM may couple to…

高能物理 - 实验 · 物理学 2025-06-24 Vindhyawasini Prasad

There is a strong possibility that the particles making up the dark matter in the Universe have a mass below 1 eV and in many important situations exhibit a wave-like behavior. Amongst the candidates the axion stands out as particularly…

高能物理 - 唯象学 · 物理学 2022-09-20 Joerg Jaeckel , Gray Rybka , Lindley Winslow

The origin of merging binary black holes detected through gravitational waves remains a fundamental question in astrophysics. While stellar evolution imposes an upper mass limit of about 50 solar mass for black holes, some observed…

高能天体物理现象 · 物理学 2025-10-03 LingQin Xue , Hiromichi Tagawa , Zoltan Haiman , Imre Bartos

We study the formation and the subsequent mass growth of axion stars inside axion miniclusters. Numerically solving the Schr\"odinger-Poisson equations with realistic initial conditions we find that the axion stars exhibit similar…

宇宙学与河外天体物理 · 物理学 2019-09-25 Benedikt Eggemeier , Jens C. Niemeyer

Axions or ALPs are hypothetical particles predicted by BSM theories, which make one of the dark matter candidates. These particles can convert into photons and vice-versa in the presence of magnetic field, with a probability decided by its…

宇宙学与河外天体物理 · 物理学 2024-09-19 Harsh Mehta , Suvodip Mukherjee

Galaxy mergers are hugely important in our current dark matter cosmology. These powerful events cause the disruption of the merging galaxies, pushing the gas, stars and dust of the galaxies resulting in changes to morphologies. This…

星系天体物理 · 物理学 2023-02-23 W. J. Pearson , L. E. Suelves , S. C. -C. Ho , N. Oi , NEP Team , GAMA Team

The potential to detect axion dark matter through astrophysical processes has shown high promise in recent years. We therefore expand on previous work studying the axion-to-photon conversion efficacy of neutron stars and the interstellar…

高能天体物理现象 · 物理学 2026-05-15 Felix Weber , Vikram Ravi

Non-linear effects in the evolution of the axion field in the early Universe may lead to the formation of gravitationally bound clumps of axions, known as "miniclusters". Minicluster masses should be in the range $M_{\rm mc}\sim10^{-12}…

高能天体物理现象 · 物理学 2015-06-23 Igor I. Tkachev

The first Advanced LIGO observing run detected two black hole merger events with confidence and likely a third. Many groups organized to followup the events in the optical even though the strong theoretical prior that no optical emission…

天体物理仪器与方法 · 物理学 2016-10-03 James Annis , Marcelle Soares-Santos

We compare new maps of the hot gas, dark matter, and galaxies for 1E0657-56, a cluster with a rare, high-velocity merger occurring nearly in the plane of the sky. The X-ray observations reveal a bullet-like gas subcluster just exiting the…

天体物理学 · 物理学 2009-11-10 M. Markevitch , A. H. Gonzalez , D. Clowe , A. Vikhlinin , L. David , W. Forman , C. Jones , S. Murray , W. Tucker

Axion dark matter passing through the magnetospheres of magnetars can undergo hyper-efficient resonant mixing with low-energy photons, leading to the production of narrow spectral lines that could be detectable on Earth. Since this is a…

高能物理 - 唯象学 · 物理学 2025-05-28 Sandip Roy , Anirudh Prabhu , Christopher Thompson , Samuel J. Witte , Carlos Blanco , Jonathan Zhang

In all supersymmetric theories, gravitinos, with mass suppressed by the Planck scale, are an obvious candidate for dark matter; but if gravitinos ever reached thermal equilibrium, such dark matter is apparently either too abundant or too…

高能物理 - 唯象学 · 物理学 2017-08-03 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall , Keisuke Harigaya