4.4 Article

Signatures for quark matter from multi-messenger observations

出版社

IOP Publishing Ltd
DOI: 10.1088/1361-6471/ab337a

关键词

neutron stars; quark matter; phase transition; nuclear astrophysics; gravitational waves

资金

  1. US Department of Energy, Office of Science, Office of Nuclear Physics [DE-FG02-05ER41375]
  2. Turkish Research Council TUBITAK [117F312]
  3. National Science Foundation [PHY-1630782]
  4. Heising-Simons Foundation [2017-228]

向作者/读者索取更多资源

We review the prospects for detecting quark matter in neutron star cores. We survey the proposed signatures and emphasize the importance of data from neutron star mergers, which provide access to dynamical properties that operate on short timescales that are not probed by most other neutron star observables.

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