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Axion dark matter (DM) produces echo images of bright radio sources via stimulated decay. These images appear as a faint radio line centered at half the axion mass, with the line width set by the DM velocity dispersion. Due to the…

高能物理 - 唯象学 · 物理学 2023-10-09 Yitian Sun , Katelin Schutz , Harper Sewalls , Calvin Leung , Kiyoshi Wesley Masui

Unexpected astrophysical observations can be explained by gravitationally captured massive particles, which are produced inside the Sun or other Stars and are accumulated over cosmic times. Their radiative decay in solar outer space would…

天体物理学 · 物理学 2009-11-07 L. DiLella , K. Zioutas

Axions provide a natural and well-motivated dark matter candidate, with the capability to convert directly to photons in the presence of an electromagnetic field. A particularly compelling observational target is the conversion of dark…

A series of dynamical anomalies in the orbits of distant trans-Neptunian objects points to a new celestial body (usually named Planet Nine) in the solar system. In this draft, we point out that a mirror planet captured from the outer solar…

地球与行星天体物理 · 物理学 2022-10-11 Pei Wang , Yu Chen Tang , Lei Zu , Yuan Yuan Chen , Lei Feng

We show that axion dark matter (DM) may be detectable through narrow radio lines emitted from neutron stars. The neutron star magnetosphere hosts a strong magnetic field and a plasma frequency that increases towards the neutron star…

高能物理 - 唯象学 · 物理学 2018-12-19 Anson Hook , Yonatan Kahn , Benjamin R. Safdi , Zhiquan Sun

We study the radio signals generated when an axion star enters the magnetosphere of a neutron star. As the axion star moves through the resonant region where the plasma-induced photon mass becomes equal to the axion mass, the axions can…

高能天体物理现象 · 物理学 2021-02-25 James H. Buckley , P. S. Bhupal Dev , Francesc Ferrer , Fa Peng Huang

Electromagnetic radiation with angular frequency equal to half the axion mass stimulates the decay of cold dark matter axions and produces an echo, i.e. faint electromagnetic radiation traveling in the opposite direction. We propose to…

高能物理 - 唯象学 · 物理学 2019-10-02 Ariel Arza , Pierre Sikivie

The search for exoplanetary radio emission has resulted in zero conclusive detections to date. Various explanations for this have been proposed, from the observed frequency range, telescope sensitivity, to beaming of the emission. In a…

太阳与恒星天体物理 · 物理学 2020-02-19 R. D. Kavanagh , A. A. Vidotto

The axion is a hypothetical elementary particle and a cold dark matter candidate. It could dominate potential wells of most astrophysical objects. Axions spontaneously decay into nearly monochromatic microwave photons. We present results…

天体物理学 · 物理学 2009-10-31 B. D. Blout , E. J. Daw , M. P. Decowski , Paul T. P. Ho , L. J Rosenberg , D. B. Yu

Axion as one of the promising dark matter candidates can be detected through narrow radio lines emitted from the magnetic white dwarf stars. Due to the existence of the strong magnetic field, the axion may resonantly convert into the radio…

高能物理 - 唯象学 · 物理学 2021-06-23 Jin-Wei Wang , Xiao-Jun Bi , Run-Min Yao , Peng-Fei Yin

As many as $10^9$ neutron stars populate the Galaxy, but only $\approx 10^3$ are directly observed as pulsars or as accreting sources in X-ray binaries. In principle also the accretion of the interstellar medium may make isolated neutron…

天体物理学 · 物理学 2009-10-31 Aldo Treves , Roberto Turolla , Silvia Zane , Monica Colpi

It has been suggested that radio telescopes may be sensitive to axion dark matter that resonantly converts to radio photons in the magnetospheres surrounding neutron stars (NSs). In this work, we closely examine this possibility by…

宇宙学与河外天体物理 · 物理学 2019-07-03 Benjamin R. Safdi , Zhiquan Sun , Alexander Y. Chen

A small admixture of dark matter gravitationally bound to the proto-Solar gas cloud could be adiabatically contracted into Earth-crossing orbits with a local density comparable to (or even exceeding) the Galactic halo density. We show that…

高能物理 - 唯象学 · 物理学 2020-07-23 Noah B. Anderson , Angelina Partenheimer , Timothy D. Wiser

Axions may make a significant contribution to the dark matter of the universe. It has been suggested that these dark matter axions may condense into localized clumps, called "axion stars." In this paper we argue that collisions of dilute…

高能物理 - 唯象学 · 物理学 2016-12-09 Stuart Raby

In a previous work we investigated the propagation of fast moving charged particles in a spatially constant but slowly time dependent pseudoscalar background, such as the one provided by cold relic axions. The background induces cosmic rays…

高能物理 - 唯象学 · 物理学 2015-03-17 D. Espriu , F. Mescia , A. Renau

The conversion of neutron matter into strange matter in a neutron star occurs through the non-leptonic weak-interaction process. We study the energy loss of the neutron star by the emission of axions in that process. Owing to that process,…

天体物理学 · 物理学 2009-10-30 In-Saeng Suh , Chul H. Lee

In the past decade, numerical simulations started to reveal the possible existence of planet 9 in our solar system. The planet 9 scenario can provide an excellent explanation to the clustering in orbital elements for Kuiper Belt objects.…

地球与行星天体物理 · 物理学 2023-06-06 Man Ho Chan

A prominent aspect of the hunt for cold dark matter is looking for light scalar candidates such as axion-like particles (ALPs). The coupling between ALPs and photons allows for the spontaneous decay of ALPs into pairs of photons. It has…

高能天体物理现象 · 物理学 2022-03-08 Ahmed Ayad , Geoff Beck

As a well-motivated dark matter candidate, axions can be detected through the axion-photon resonant conversion in the magnetospheres of magnetic white dwarf stars or neutron stars. In this work, we utilize Omega Centauri, which is the…

高能天体物理现象 · 物理学 2021-11-24 Jin-Wei Wang , Xiao-Jun Bi , Peng-Fei Yin

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.…

高能物理 - 唯象学 · 物理学 2023-03-29 Samuel J. Witte , Sebastian Baum , Matthew Lawson , M. C. David Marsh , Alexander J. Millar , Gustavo Salinas