D
Dany Page
Researcher at National Autonomous University of Mexico
Publications - 141
Citations - 6460
Dany Page is an academic researcher from National Autonomous University of Mexico. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 38, co-authored 138 publications receiving 5869 citations. Previous affiliations of Dany Page include Joint Institute for Nuclear Astrophysics & Stony Brook University.
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Minimal Cooling of Neutron Stars: A New Paradigm
TL;DR: In this paper, a new classification of neutron star cooling scenarios, involving either "minimal" cooling or "enhanced" cooling, is proposed, which is distinguished from enhanced cooling by the absence of neutrino emission from any direct Urca process, due either to nucleons or to exotica such as hyperons or deconfined quarks.
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Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense Matter
TL;DR: This work proposes that the observed cooling of the neutron star in Cassiopeia A is due to enhanced neutrino emission from the recent onset of the breaking and formation of neutron Cooper pairs in the (3)P(2) channel and finds the critical temperature for this superfluid transition is ≃0.5×10(9) K.
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The cooling of compact stars
TL;DR: The cooling of a compact star depends very sensitively on the state of matter at supranuclear densities, which essentially controls the neutrino emission, as well as on the structure of the stellar outer layers which control the photon emission as mentioned in this paper.
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Neutron Stars—Cooling and Transport
TL;DR: In this paper, the basics of thermal evolution for isolated neutron stars with strong magnetic fields are reviewed, including most relevant thermodynamic and kinetic properties in the stellar core, crust, and blanketing envelopes.
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Dense Matter in Compact Stars: Theoretical Developments and Observational Constraints
Dany Page,Sanjay Reddy +1 more
TL;DR: In this article, theoretical developments in studies of dense matter and its phase structure of relevance to compact stars are reviewed, and observations on compact stars, which can constrain the properties of dense dense matter, are presented critically and interpreted.