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Title: QCD axion star collapse with the chiral potential

Abstract

In a previous study, we analyzed collapsing axion stars using the low-energy instanton potential, showing that the total energy is always bounded and that collapsing axion stars do not form black holes. In this paper, we provide a proof that the conclusions are unchanged when using instead the more general chiral potential for QCD axions.

Authors:
 [1];  [2];  [2];  [2]
  1. Univ. of Cincinnati, Cincinnati, OH (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  2. Univ. of Cincinnati, Cincinnati, OH (United States)
Publication Date:
Research Org.:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
OSTI Identifier:
1346356
Report Number(s):
arXiv:1702.05504; FERMILAB-PUB-17-056-T
Journal ID: ISSN 1029-8479; 1514262
Grant/Contract Number:  
AC02-07CH11359
Resource Type:
Accepted Manuscript
Journal Name:
Journal of High Energy Physics (Online)
Additional Journal Information:
Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2017; Journal Issue: 6; Journal ID: ISSN 1029-8479
Publisher:
Springer Berlin
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; classical theories of gravity; cosmology of theories beyond the SM

Citation Formats

Eby, Joshua, Leembruggen, Madelyn, Suranyi, Peter, and Wijewardhana, L. C. R. QCD axion star collapse with the chiral potential. United States: N. p., 2017. Web. doi:10.1007/JHEP06(2017)014.
Eby, Joshua, Leembruggen, Madelyn, Suranyi, Peter, & Wijewardhana, L. C. R. QCD axion star collapse with the chiral potential. United States. doi:10.1007/JHEP06(2017)014.
Eby, Joshua, Leembruggen, Madelyn, Suranyi, Peter, and Wijewardhana, L. C. R. Mon . "QCD axion star collapse with the chiral potential". United States. doi:10.1007/JHEP06(2017)014. https://www.osti.gov/servlets/purl/1346356.
@article{osti_1346356,
title = {QCD axion star collapse with the chiral potential},
author = {Eby, Joshua and Leembruggen, Madelyn and Suranyi, Peter and Wijewardhana, L. C. R.},
abstractNote = {In a previous study, we analyzed collapsing axion stars using the low-energy instanton potential, showing that the total energy is always bounded and that collapsing axion stars do not form black holes. In this paper, we provide a proof that the conclusions are unchanged when using instead the more general chiral potential for QCD axions.},
doi = {10.1007/JHEP06(2017)014},
journal = {Journal of High Energy Physics (Online)},
number = 6,
volume = 2017,
place = {United States},
year = {2017},
month = {6}
}

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Cited by: 3 works
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    Works referencing / citing this record:

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