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...
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| Formato: | Online |
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| Idioma: | inglês |
| Publicado em: |
MDPI - Multidisciplinary Digital Publishing Institute
2024
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| Acesso em linha: | ONIX_20240906_9783725815999_125 |
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| _version_ | 1869517458838126592 |
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| collection | Directory of Open Access Books |
| description | 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 system, has opened a new window to explore the physics of neutron stars. The following Special Issue is a collection of various contributions dedicated to modern applications of the theory of nuclear matter in neutron stars and its main purpose is to shed light on some of the open problems concerning the nuclear physics of neutron stars and how they can possibly be addressed or even answered. |
| format | Online |
| id | doab-20.500.12854ir-143763 |
| institution | Directory of Open Access Books |
| language | eng |
| publishDate | 2024 |
| publishDateRange | 2024 |
| publishDateSort | 2024 |
| publisher | MDPI - Multidisciplinary Digital Publishing Institute |
| publisherStr | MDPI - Multidisciplinary Digital Publishing Institute |
| record_format | ojs |
| spelling | doab-20.500.12854ir-1437632024-09-06T08:20:16Z The Nuclear Physics of Neutron Stars Moustakidis, Charalampos 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 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 system, has opened a new window to explore the physics of neutron stars. The following Special Issue is a collection of various contributions dedicated to modern applications of the theory of nuclear matter in neutron stars and its main purpose is to shed light on some of the open problems concerning the nuclear physics of neutron stars and how they can possibly be addressed or even answered. 2024-09-06T08:20:10Z 2024-09-06T08:20:10Z 2024 book ONIX_20240906_9783725815999_125 9783725815999 9783725816002 https://directory.doabooks.org/handle/20.500.12854/143763 eng application/octet-stream Attribution-NonCommercial-NoDerivatives 4.0 International https://mdpi.com/books/pdfview/book/9492 https://mdpi.com/books/pdfview/book/9492 MDPI - Multidisciplinary Digital Publishing Institute 10.3390/books978-3-7258-1600-2 10.3390/books978-3-7258-1600-2 46cabcaa-dd94-4bfe-87b4-55023c1b36d0 9783725815999 9783725816002 open access |
| spellingShingle | 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 The Nuclear Physics of Neutron Stars |
| title | The Nuclear Physics of Neutron Stars |
| title_full | The Nuclear Physics of Neutron Stars |
| title_fullStr | The Nuclear Physics of Neutron Stars |
| title_full_unstemmed | The Nuclear Physics of Neutron Stars |
| title_short | The Nuclear Physics of Neutron Stars |
| title_sort | nuclear physics of neutron stars |
| topic | 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 |
| topic_facet | 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 |
| url | ONIX_20240906_9783725815999_125 |