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The Nuclear Physics of Neutron Stars

Neutron stars are considered extraordinary astronomical laboratories for the physics of nuclear matter as they have the most fascinating constitution of energy and matter in the universe. Recently, the detection of gravitational waves from the merger of two neutron stars, in a binary neutron star sy...

Täydet tiedot

Tallennettuna:
Aineistotyyppi: Online
Kieli:englanti
Julkaistu: MDPI - Multidisciplinary Digital Publishing Institute 2024
Aiheet:
equation of state
neutron star
GW190814
maximum mass
tidal deformability
nuclear matter
gravitational waves
binary mergers
unified equation of state
Gogny interaction
symmetry energy
moment of inertia
neutron stars
scalar-tensor gravity
Higgs inflationary model
XRBs
astrophysical jets
photo-pion production
extragalactic
γ-ray emission
lepto-hadronic model
topology for baryons
hidden symmetries
ultra dense matter
compact stars
X17
EoS
Massive compact stars
topology change
hadron-quark continuity
Cheshire Cat Principle
hidden symmetries dual to gluons
GnEFT
psuedo-conformality
nuclear matter saturation properties
landau parameters
incompressibility of nuclear matter
neutron star properties
binary neutron star merger
gravitational redshift
relativistic fluids
interior solutions
spherically symmetric sources
n/a
thema EDItEUR::P Mathematics and Science
thema EDItEUR::P Mathematics and Science::PH Physics
thema EDItEUR::P Mathematics and Science::PH Physics::PHN Nuclear physics
Linkit:ONIX_20240906_9783725815999_125
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ONIX_20240906_9783725815999_125

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