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Dense Matter in Compact Stars: Theoretical Developments and Observational Constraints

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arxiv astro-ph/0608360 v1 pith:5HE67A3T submitted 2006-08-17 astro-ph hep-phnucl-th

Dany Page (1) , Sanjay Reddy (2) ((1) Instituto de Astronomia , UNAM , Mexico , (2) Theoretical Division , Los Alamos National Laboratory , USA) This is my paper · ORCID
classification astro-phhep-phnucl-th
keywords compactdensematterstarsdevelopmentsobservationaltheoreticalconstrain
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We review theoretical developments in studies of dense matter and its phase structure of relevance to compact stars. Observational data on compact stars, which can constrain the properties of dense matter, are presented critically and interpreted.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. On the Nucleon Effective Mass in Neutron Stars Cooling

    hep-th 2026-07 conditional novelty 6.0 of 10

    Using the Landau instead of the Dirac effective nucleon mass in neutron-star cooling calculations cools massive stars faster, changing predicted surface temperatures by ~0.03–0.06 dex.

  2. New Gauge Forces, Neutron Stars and Schwinger Neutrino Production

    hep-ph 2026-06 unverdicted novelty 5.0 of 10

    For Lμ-Lτ gauge forces with g ≳ 10^{-18}, Schwinger neutrino production in neutron stars alters composition, invalidates merger constraints at g ≳ 10^{-17}, and could yield detectable ~100 MeV neutrino fluxes from you...

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