Weak and electromagnetic mechanisms of neutrino-pair photoproduction in a strongly magnetized electron gas
Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Borisov, A. V. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2012 |
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| Schlagwörter: |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2012 |
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| Übergeordnetes Werk: |
Enthalten in: Physics of atomic nuclei - SP MAIK Nauka/Interperiodica, 1993, 75(2012), 11 vom: Nov., Seite 1305-1312 |
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| Übergeordnetes Werk: |
volume:75 ; year:2012 ; number:11 ; month:11 ; pages:1305-1312 |
| Links: |
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| DOI / URN: |
10.1134/S1063778812110051 |
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OLC2049918488 |
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| 520 | |a Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. | ||
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| 700 | 1 | |a Sizin, P. E. |4 aut | |
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10.1134/S1063778812110051 doi (DE-627)OLC2049918488 (DE-He213)S1063778812110051-p DE-627 ger DE-627 rakwb eng 530 VZ Borisov, A. V. verfasserin aut Weak and electromagnetic mechanisms of neutrino-pair photoproduction in a strongly magnetized electron gas 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. Neutron Star Atomic Nucleus Compton Scattering Magnetic Dipole Moment Electromagnetic Form Factor Kerimov, B. K. aut Sizin, P. E. aut Enthalten in Physics of atomic nuclei SP MAIK Nauka/Interperiodica, 1993 75(2012), 11 vom: Nov., Seite 1305-1312 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:75 year:2012 number:11 month:11 pages:1305-1312 https://doi.org/10.1134/S1063778812110051 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 75 2012 11 11 1305-1312 |
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10.1134/S1063778812110051 doi (DE-627)OLC2049918488 (DE-He213)S1063778812110051-p DE-627 ger DE-627 rakwb eng 530 VZ Borisov, A. V. verfasserin aut Weak and electromagnetic mechanisms of neutrino-pair photoproduction in a strongly magnetized electron gas 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. Neutron Star Atomic Nucleus Compton Scattering Magnetic Dipole Moment Electromagnetic Form Factor Kerimov, B. K. aut Sizin, P. E. aut Enthalten in Physics of atomic nuclei SP MAIK Nauka/Interperiodica, 1993 75(2012), 11 vom: Nov., Seite 1305-1312 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:75 year:2012 number:11 month:11 pages:1305-1312 https://doi.org/10.1134/S1063778812110051 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 75 2012 11 11 1305-1312 |
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10.1134/S1063778812110051 doi (DE-627)OLC2049918488 (DE-He213)S1063778812110051-p DE-627 ger DE-627 rakwb eng 530 VZ Borisov, A. V. verfasserin aut Weak and electromagnetic mechanisms of neutrino-pair photoproduction in a strongly magnetized electron gas 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. Neutron Star Atomic Nucleus Compton Scattering Magnetic Dipole Moment Electromagnetic Form Factor Kerimov, B. K. aut Sizin, P. E. aut Enthalten in Physics of atomic nuclei SP MAIK Nauka/Interperiodica, 1993 75(2012), 11 vom: Nov., Seite 1305-1312 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:75 year:2012 number:11 month:11 pages:1305-1312 https://doi.org/10.1134/S1063778812110051 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 75 2012 11 11 1305-1312 |
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10.1134/S1063778812110051 doi (DE-627)OLC2049918488 (DE-He213)S1063778812110051-p DE-627 ger DE-627 rakwb eng 530 VZ Borisov, A. V. verfasserin aut Weak and electromagnetic mechanisms of neutrino-pair photoproduction in a strongly magnetized electron gas 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. Neutron Star Atomic Nucleus Compton Scattering Magnetic Dipole Moment Electromagnetic Form Factor Kerimov, B. K. aut Sizin, P. E. aut Enthalten in Physics of atomic nuclei SP MAIK Nauka/Interperiodica, 1993 75(2012), 11 vom: Nov., Seite 1305-1312 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:75 year:2012 number:11 month:11 pages:1305-1312 https://doi.org/10.1134/S1063778812110051 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 75 2012 11 11 1305-1312 |
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10.1134/S1063778812110051 doi (DE-627)OLC2049918488 (DE-He213)S1063778812110051-p DE-627 ger DE-627 rakwb eng 530 VZ Borisov, A. V. verfasserin aut Weak and electromagnetic mechanisms of neutrino-pair photoproduction in a strongly magnetized electron gas 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. Neutron Star Atomic Nucleus Compton Scattering Magnetic Dipole Moment Electromagnetic Form Factor Kerimov, B. K. aut Sizin, P. E. aut Enthalten in Physics of atomic nuclei SP MAIK Nauka/Interperiodica, 1993 75(2012), 11 vom: Nov., Seite 1305-1312 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:75 year:2012 number:11 month:11 pages:1305-1312 https://doi.org/10.1134/S1063778812110051 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 75 2012 11 11 1305-1312 |
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Weak and electromagnetic mechanisms of neutrino-pair photoproduction in a strongly magnetized electron gas |
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Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. © Pleiades Publishing, Ltd. 2012 |
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Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. © Pleiades Publishing, Ltd. 2012 |
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Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained. © Pleiades Publishing, Ltd. 2012 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2049918488</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504110546.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2012 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1134/S1063778812110051</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2049918488</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)S1063778812110051-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Borisov, A. V.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Weak and electromagnetic mechanisms of neutrino-pair photoproduction in a strongly magnetized electron gas</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2012</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Pleiades Publishing, Ltd. 2012</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Expressions for the power of neutrino radiation from a degenerate electron gas in a strong magnetic field are derived for the case of neutrino-pair photoproduction via the weak and electromagnetic interaction mechanisms (it is assumed that the neutrino possesses electromagnetic form factors). It is shown that the neutrino luminosity of a medium in the electromagnetic reaction channel may exceed substantially the luminosity in the weak channel. Relative upper bounds on the effective neutrino magnetic moment are obtained.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Neutron Star</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Atomic Nucleus</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Compton Scattering</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Magnetic Dipole Moment</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Electromagnetic Form Factor</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kerimov, B. K.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sizin, P. E.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Physics of atomic nuclei</subfield><subfield code="d">SP MAIK Nauka/Interperiodica, 1993</subfield><subfield code="g">75(2012), 11 vom: Nov., Seite 1305-1312</subfield><subfield code="w">(DE-627)131188437</subfield><subfield code="w">(DE-600)1146378-8</subfield><subfield code="w">(DE-576)032622155</subfield><subfield code="x">1063-7788</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:75</subfield><subfield code="g">year:2012</subfield><subfield code="g">number:11</subfield><subfield code="g">month:11</subfield><subfield code="g">pages:1305-1312</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1134/S1063778812110051</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">75</subfield><subfield code="j">2012</subfield><subfield code="e">11</subfield><subfield code="c">11</subfield><subfield code="h">1305-1312</subfield></datafield></record></collection>
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