Cooling of hypernuclear compact stars
arXiv:1712.00584 · doi:10.1093/mnras/stx3318
Abstract
We study the thermal evolution of hypernuclear compact stars constructed from covariant density functional theory of hypernuclear matter and parameterizations which produce sequences of stars containing two-solar-mass objects. For the input in the simulations, we solve the Bardeen-Cooper-Schrieffer gap equations in the hyperonic sector and obtain the gaps in the spectra of , and hyperons. For the models with masses the neutrino cooling is dominated by hyperonic direct Urca processes in general. In the low-mass stars the plus leptons channel is the dominant direct Urca process, whereas for more massive stars the purely hyperonic channels and are dominant. Hyperonic pairing strongly suppresses the processes on s and to a lesser degree on s. We find that intermediate-mass models have surface temperatures which lie within the range inferred from thermally emitting neutron stars, if the hyperonic pairing is taken into account. Most massive models with may cool very fast via the direct Urca process through the channel because they develop inner cores where the -wave pairing of s and proton is absent.
v2: minor changes, matches published version, 11 pages, 9 figures
References in corpus (16)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- Constraints on the Symmetry Energy Using the Mass-Radius Relation of Neutron Stars
- Pulsars as Astrophysical Laboratories for Nuclear and Particle Physics
- Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints
- A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations
- Constraining hypernuclear density functional with -hypernuclei and compact stars
- Neutrino emission due to Cooper-pair recombination in neutron stars revisited
- Statistical theory of thermal evolution of neutron stars
- A Massive Millisecond Pulsar in an Eccentric Binary
- Many-body forces in the equation of state of hyperonic matter
- Vertex renormalization in weak decays of Cooper pairs and cooling compact stars
- Superfluid Response and the Neutrino Emissivity of Neutron Matter
- BCS-BEC crossovers and unconventional phases in dilute nuclear matter
- Maximal isospin few-body systems of nucleons and hyperons
- Theory of neutrino emission from nucleon-hyperon matter in neutron stars: Angular integrals
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