Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma
The cardinal focus of the present review is to explore the role of neutrinos originating from the ultradense core of neutron stars composed of quark gluon plasma in the astrophysical scenario. The collective excitations of the quarks involving the neutrinos through the different kinematical processe...
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| Format: | Article |
| Language: | English |
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Wiley
2017-01-01
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| Series: | Advances in High Energy Physics |
| Online Access: | http://dx.doi.org/10.1155/2017/1273931 |
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| author | Souvik Priyam Adhya |
| author_facet | Souvik Priyam Adhya |
| author_sort | Souvik Priyam Adhya |
| collection | DOAJ |
| description | The cardinal focus of the present review is to explore the role of neutrinos originating from the ultradense core of neutron stars composed of quark gluon plasma in the astrophysical scenario. The collective excitations of the quarks involving the neutrinos through the different kinematical processes have been studied. The cooling of the neutron stars as well as pulsar kicks due to asymmetric neutrino emission has been discussed in detail. Results involving calculation of relevant physical quantities like neutrino mean free path and emissivity have been presented in the framework of non-Fermi liquid behavior as applicable to ultradegenerate plasma. |
| format | Article |
| id | doaj-art-470f3abb13bf45b7a112933245cd4d2b |
| institution | Kabale University |
| issn | 1687-7357 1687-7365 |
| language | English |
| publishDate | 2017-01-01 |
| publisher | Wiley |
| record_format | Article |
| series | Advances in High Energy Physics |
| spelling | doaj-art-470f3abb13bf45b7a112933245cd4d2b2025-02-03T06:08:47ZengWileyAdvances in High Energy Physics1687-73571687-73652017-01-01201710.1155/2017/12739311273931Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon PlasmaSouvik Priyam Adhya0Experimental High Energy Physics and Applications Group, Variable Energy Cyclotron Center, 1/AF Bidhannagar, Kolkata 700 064, IndiaThe cardinal focus of the present review is to explore the role of neutrinos originating from the ultradense core of neutron stars composed of quark gluon plasma in the astrophysical scenario. The collective excitations of the quarks involving the neutrinos through the different kinematical processes have been studied. The cooling of the neutron stars as well as pulsar kicks due to asymmetric neutrino emission has been discussed in detail. Results involving calculation of relevant physical quantities like neutrino mean free path and emissivity have been presented in the framework of non-Fermi liquid behavior as applicable to ultradegenerate plasma.http://dx.doi.org/10.1155/2017/1273931 |
| spellingShingle | Souvik Priyam Adhya Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma Advances in High Energy Physics |
| title | Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma |
| title_full | Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma |
| title_fullStr | Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma |
| title_full_unstemmed | Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma |
| title_short | Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma |
| title_sort | astrophysical aspects of neutrino dynamics in ultradegenerate quark gluon plasma |
| url | http://dx.doi.org/10.1155/2017/1273931 |
| work_keys_str_mv | AT souvikpriyamadhya astrophysicalaspectsofneutrinodynamicsinultradegeneratequarkgluonplasma |