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Isolated Neutron Stars
Non-accreting neutron stars display diverse characteristics, leading us to classify them into several groups. This chapter is an observational driven... -
Isolated Neutron Stars
Non-accreting neutron stars display diverse characteristics, leading us to classify them into several groups. This chapter is an observational driven... -
Neutron Stars
Neutron stars are highly compact astrophysical objects and therefore of utmost relevance to learn about theories of gravity. Whereas the proper... -
Fundamental Physics with Neutron Stars
Neutron stars are rich laboratories of multiple branches of modern physics. These include gravitational physics, nuclear and particle physics,... -
Electrobaryonic axion: hair of neutron stars
Axion-like particles are predicted in many physics scenarios beyond the Standard Model (SM). Their interactions with SM particles may arise from the...
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Effects of dark matter on the spontaneous scalarization in neutron stars
Dark matter, an important portion of compact objects, can influence different phenomena in neutron stars. The spontaneous scalarization in the...
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Scalarized hybrid neutron stars in scalar tensor gravity
Hybrid neutron stars, the compact objects consisting hadronic matter and strange quark matter, can be considered as the probes for the scalar tensor...
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Skyrme-Like Λ Hyperonic Interactions and Neutron Stars Properties
AbstractAt high densities that are achieved in neutron stars, there may be additional sensitivity to certain properties of the baryonic interaction....
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Neutron Stars as Extreme Gravity Probes
Neutron stars are powerful probes into the extremes of physics. In this chapter, we will discuss how observations of neutron stars, either in... -
Neutron stars in the Witten-Sakai-Sugimoto model
We utilize the top-down holographic QCD model, the Witten-Sakai-Sugimoto model, in a hybrid setting with the SLy4, soft chiral EFT and stiff chiral...
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Neutron Stars and Black Holes as Natural Laboratories of Fundamental Physics
AbstractThe statistics of particles with half-integer spin was constructed in 1926 in the works of E. Fermi and P. A. M. Dirac. Soon after, it was...
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Spontaneous scalarization in proto-neutron stars
Proto-neutron stars are born when a highly evolved and massive star collapses under gravity. In this paper, we investigate the spontaneous...
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Quantum vortices in fermionic superfluids: from ultracold atoms to neutron stars.
Superfluid dilute neutron matter and ultracold gas, close to the unitary regime, exhibit several similarities. Therefore, to a certain extent,...
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Constraints on the dense matter equation of state from young and cold isolated neutron stars
Neutron stars are the dense and highly magnetic relics of supernova explosions of massive stars. The quest to constrain the equation of state (EOS)...
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A constraint on the dissipative tidal deformability of neutron stars
The gravitational waves emitted by neutron star binaries probe the physics of matter at supranuclear densities. During the late inspiral, tidal...
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Fundamental Physics with Neutron Stars
Neutron stars are rich laboratories of multiple branches of modern physics. These include gravitational physics, nuclear and particle physics,... -
Hypernuclei and Neutron Stars with Charge Symmetry Breaking Hyperonic Potential
AbstractIn this paper, we propose a method of taking charge symmetry breaking (CSB) in hypernuclei and neutron stars into account within the...
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Gapless neutron superfluidity in the crust of the accreting neutron stars KS 1731−260 and MXB 1659−29
The interpretation of the thermal evolution of the transiently accreting neutron stars MXB 1659−29 and KS 1731−260 after an outburst is challenging,...
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Quasi-periodic sub-pulse structure as a unifying feature for radio-emitting neutron stars
Magnetars are highly magnetized rotating neutron stars that are predominantly observed as high-energy sources. Six of this class of neutron star are...
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Equation of State of Hypernuclear Matter and Neutron Stars
These lectures contain a pedagogical introduction to the equation of state of nuclear matter and to the structure of neutron stars. Particular...