Axions: From magnetars and neutron star mergers to beam dumps and BECs

Author:

Fortin Jean-François1,Guo Huai-Ke2,Harris Steven P.3,Kim Doojin4,Sinha Kuver2,Sun Chen5

Affiliation:

1. Département de Physique, de Génie Physique et d’Optique, Université Laval, Québec, QC G1V 0A6, Canada

2. Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA

3. Institute for Nuclear Theory, University of Washington, Seattle, WA 98195, USA

4. Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA

5. School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 69978, Israel

Abstract

We review topics in searches for axion-like-particles (ALPs), covering material that is complementary to other recent reviews. The first half of our review covers ALPs in the extreme environments of neutron star cores, the magnetospheres of highly magnetized neutron stars (magnetars), and in neutron star mergers. The focus is on possible signals of ALPs in the photon spectrum of neutron stars and gravitational wave/electromagnetic signals from neutron star mergers. We then review recent developments in laboratory-produced ALP searches, focusing mainly on accelerator-based facilities including beam-dump type experiments and collider experiments. We provide a general-purpose discussion of the ALP search pipeline from production to detection, in steps, and our discussion is straightforwardly applicable to most beam-dump type and reactor experiments. We end with a selective look at the rapidly developing field of ultralight dark matter, specifically the formation of Bose–Einstein Condensates (BECs). We review the properties of BECs of ultralight dark matter and bridge these properties with developments in numerical simulations, and ultimately with their impact on experimental searches.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

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