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The recently discovered fast radio bursts (FRBs), presumably of extra-galactic origin, have the potential to become a powerful probe of the intergalactic medium (IGM). We point out a few such potential applications. We provide expressions…

High Energy Astrophysical Phenomena · Physics 2015-12-29 Z. Zheng , E. O. Ofek , S. R. Kulkarni , J. D. Neill , M. Juric

We have proposed a model of a progenitor of fast radio bursts (FRBs): The FRBs are emitted by electrons in atmospheres of neutron stars when neutron stars collide with dark matter axion stars. We reexamine the model by taking account of the…

High Energy Physics - Phenomenology · Physics 2015-12-22 Aiichi Iwazaki

The axion is a highly motivated elementary particle which could address two fundamental questions in physics - the strong CP problem and the dark matter mystery. Experimental searches for this hypothetical particle have started to reach…

High Energy Physics - Phenomenology · Physics 2021-10-28 Yannis K. Semertzidis , SungWoo Youn

Fast Radio Bursts (FRBs) are new transient radio sources discovered recently. Because of the angular resolution restriction in radio surveys, no optical counter part has been identified yet so it is hard to determine the progenitor of FRBs.…

High Energy Astrophysical Phenomena · Physics 2014-05-15 Chun-Yu Li , Li-Xin Li

Fast Radio Bursts (FRBs) probe baryons permeating the cosmic web through their dispersion measures (DMs), which encode the integrated electron density along cosmological sightlines. Using 3,455 unique FRB sources from CHIME/FRB with $\sim…

The axion is a light pseudoscalar particle which suppresses CP-violating effects in strong interactions and also happens to be an excellent dark matter candidate. Axions constituting the dark matter halo of our galaxy may be detected by…

In certain models of a QCD axion, finite density corrections to the axion potential can result in the axion being sourced by large dense objects. There are a variety of ways to test this phenomenon, but perhaps the most surprising effect is…

High Energy Physics - Phenomenology · Physics 2018-07-04 Anson Hook , Junwu Huang

The Hubble constant, $H_0$, is a crucial parameter in cosmology. However, various cosmic observations have produced differing posterior values for $H_0$, resulting in what is referred to as the $H_0$ tension. To resolve this discrepancy,…

High Energy Physics - Phenomenology · Physics 2024-11-25 Haoran Di , Lijing Shao , Zhu Yi , Shi-Bei Kong

Fast radio bursts can be caused by some phenomena related to 'new physics'.One of the most prominent candidates of the kind are axion Bose stars which can engender bursts when undergoing conversion into photons in magnetospheres of neutron…

High Energy Astrophysical Phenomena · Physics 2020-05-07 Maxim S. Pshirkov

If the dark matter particles are axions, gravity can cause them to coalesce into axion stars, which are stable gravitationally bound systems of axions. In the previously known solutions for axion stars, gravity and the attractive force…

High Energy Physics - Phenomenology · Physics 2016-09-20 Eric Braaten , Abhishek Mohapatra , Hong Zhang

Gravitationally bound clumps of dark matter axions in the form of 'miniclusters' or even denser 'axion stars' can generate strong radio signals through axion-photon conversion when encountering highly magnetised neutron star magnetospheres.…

High Energy Physics - Phenomenology · Physics 2023-03-29 Samuel J. Witte , Sebastian Baum , Matthew Lawson , M. C. David Marsh , Alexander J. Millar , Gustavo Salinas

We consider the possible observation of Fast Radio Bursts (FRBs) with planned future radio telescopes, and investigate how well the dispersions and redshifts of these signals might constrain cosmological parameters. We construct mock…

Cosmology and Nongalactic Astrophysics · Physics 2018-04-11 Anthony Walters , Amanda Weltman , B. M. Gaensler , Yin-Zhe Ma , Amadeus Witzemann

Axion dark matter or any ultralight bosonic dark matter can go through Bose-Einstein condensation due to the large phase density, leading to the formation of axion stars or solitons in dark matter halo centers. The formation rate is…

High Energy Physics - Phenomenology · Physics 2025-08-13 Patrick J. Fox , Neal Weiner , Huangyu Xiao

One of the most compelling candidates for Dark Matter (DM) are light pseudo-scalar particles (axions), motivated by the strong CP problem and axiverse scenario in string theory. Depending on their mass and type of self-interaction, these…

General Relativity and Quantum Cosmology · Physics 2019-07-30 Mateja Bošković

Magnetic field dependent transient solar observations are suggestive for axion-photon oscillations with light axion(-like) particle involvement. Novel dark-moon measurements with the SMART X-ray detectors can be conclusive for radiatively…

Axion dark matter (DM) is predicted to convert into radio waves in neutron star magnetospheres. We assess the detectability of this signal using a 5 m radio telescope to be installed at the Fan Mountain Observatory, operating in the UHF, L-…

We present systematic case studies to investigate the sensitivity of axion searches by liquid xenon detectors, using the axio-electric effect (analogue of the photoelectric effect) on xenon atoms. Liquid xenon is widely considered to be one…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 K. Arisaka , P. Beltrame , C. Ghag , J. Kaidi , K. Lung , A. Lyashenko , R. D. Peccei , P. Smith , K. Ye

Fast Radio Bursts (FRBs) are extragalactic millisecond-duration radio transients whose nature remains unknown. The advent of numerous facilities conducting dedicated FRB searches has dramatically revolutionised the field: hundreds of new…

High Energy Astrophysical Phenomena · Physics 2024-12-03 Inés Pastor-Marazuela

Despite existing constraints, it remains possible that up to $35\%$ of all dark matter is comprised of compact objects, such as the black holes in the 10-100\,M$_\odot$ range whose existence has been confirmed by LIGO. The strong…

Cosmology and Nongalactic Astrophysics · Physics 2020-09-10 Mawson W. Sammons , Jean-Pierre Macquart , Ron D. Ekers , Ryan M. Shannon , Hyerin Cho , J. Xavier Prochaska , Adam T. Deller , Cherie K. Day

We discuss axion dark matter detection via two mechanisms: spontaneous decays and resonant conversion in neutron star magnetospheres. For decays, we show that the brightness temperature signal, rather than flux, is a less ambiguous measure…

Cosmology and Nongalactic Astrophysics · Physics 2020-07-15 Richard A. Battye , Bjoern Garbrecht , Jamie I. McDonald , Francesco Pace , Sankarshana Srinivasan