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Resonant production of $\gamma$ rays in jolted cold neutron stars
Acoustic shock waves passing through colliding cold neutron stars can cause repetitive superconducting phase transitions in which the proton condensate relaxes to its equilibrium value via coherent oscillations. As a result, a resonant non-thermal production of gamma rays in the MeV energy range wit...
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| Lenguaje: | eng |
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1998
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| Acceso en línea: | http://cds.cern.ch/record/352078 |
| _version_ | 1780892339678478336 |
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| author | Kusenko, Alexander |
| author_facet | Kusenko, Alexander |
| author_sort | Kusenko, Alexander |
| collection | CERN |
| description | Acoustic shock waves passing through colliding cold neutron stars can cause repetitive superconducting phase transitions in which the proton condensate relaxes to its equilibrium value via coherent oscillations. As a result, a resonant non-thermal production of gamma rays in the MeV energy range with power up to 10^(52) erg/s can take place during the short period of time before the nuclear matter is heated by the shock waves. |
| id | cern-352078 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 1998 |
| record_format | invenio |
| spelling | cern-3520782023-03-14T18:46:53Zhttp://cds.cern.ch/record/352078engKusenko, AlexanderResonant production of $\gamma$ rays in jolted cold neutron starsAstrophysics and AstronomyAcoustic shock waves passing through colliding cold neutron stars can cause repetitive superconducting phase transitions in which the proton condensate relaxes to its equilibrium value via coherent oscillations. As a result, a resonant non-thermal production of gamma rays in the MeV energy range with power up to 10^(52) erg/s can take place during the short period of time before the nuclear matter is heated by the shock waves.Acoustic shock waves passing through colliding cold neutron stars can cause repetitive superconducting phase transitions in which the proton condensate relaxes to its equilibrium value via coherent oscillations. As a result, a resonant non-thermal production of gamma rays in the MeV energy range with power up to 10^(52) erg/s can take place during the short period of time before the nuclear matter is heated by the shock waves.astro-ph/9804134CERN-TH-98-125CERN-TH-98-125oai:cds.cern.ch:3520781998-04-15 |
| spellingShingle | Astrophysics and Astronomy Kusenko, Alexander Resonant production of $\gamma$ rays in jolted cold neutron stars |
| title | Resonant production of $\gamma$ rays in jolted cold neutron stars |
| title_full | Resonant production of $\gamma$ rays in jolted cold neutron stars |
| title_fullStr | Resonant production of $\gamma$ rays in jolted cold neutron stars |
| title_full_unstemmed | Resonant production of $\gamma$ rays in jolted cold neutron stars |
| title_short | Resonant production of $\gamma$ rays in jolted cold neutron stars |
| title_sort | resonant production of $\gamma$ rays in jolted cold neutron stars |
| topic | Astrophysics and Astronomy |
| url | http://cds.cern.ch/record/352078 |
| work_keys_str_mv | AT kusenkoalexander resonantproductionofgammaraysinjoltedcoldneutronstars |