Nonthermal radiation from black holes
Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole....
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Khriplovich, I. B. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2002 |
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| Schlagwörter: |
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| Anmerkung: |
© MAIK "Nauka/Interperiodica" 2002 |
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| Übergeordnetes Werk: |
Enthalten in: Physics of atomic nuclei - Nauka/Interperiodica, 1993, 65(2002), 7 vom: Juli, Seite 1259-1270 |
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| Übergeordnetes Werk: |
volume:65 ; year:2002 ; number:7 ; month:07 ; pages:1259-1270 |
| Links: |
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| DOI / URN: |
10.1134/1.1495025 |
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OLC2049894368 |
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| 520 | |a Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. | ||
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10.1134/1.1495025 doi (DE-627)OLC2049894368 (DE-He213)1.1495025-p DE-627 ger DE-627 rakwb eng 530 VZ Khriplovich, I. B. verfasserin aut Nonthermal radiation from black holes 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2002 Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. Radiation Black Hole Elementary Particle Particle Production Charged Black Hole Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 65(2002), 7 vom: Juli, Seite 1259-1270 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:65 year:2002 number:7 month:07 pages:1259-1270 https://doi.org/10.1134/1.1495025 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2279 AR 65 2002 7 07 1259-1270 |
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10.1134/1.1495025 doi (DE-627)OLC2049894368 (DE-He213)1.1495025-p DE-627 ger DE-627 rakwb eng 530 VZ Khriplovich, I. B. verfasserin aut Nonthermal radiation from black holes 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2002 Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. Radiation Black Hole Elementary Particle Particle Production Charged Black Hole Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 65(2002), 7 vom: Juli, Seite 1259-1270 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:65 year:2002 number:7 month:07 pages:1259-1270 https://doi.org/10.1134/1.1495025 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2279 AR 65 2002 7 07 1259-1270 |
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10.1134/1.1495025 doi (DE-627)OLC2049894368 (DE-He213)1.1495025-p DE-627 ger DE-627 rakwb eng 530 VZ Khriplovich, I. B. verfasserin aut Nonthermal radiation from black holes 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2002 Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. Radiation Black Hole Elementary Particle Particle Production Charged Black Hole Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 65(2002), 7 vom: Juli, Seite 1259-1270 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:65 year:2002 number:7 month:07 pages:1259-1270 https://doi.org/10.1134/1.1495025 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2279 AR 65 2002 7 07 1259-1270 |
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10.1134/1.1495025 doi (DE-627)OLC2049894368 (DE-He213)1.1495025-p DE-627 ger DE-627 rakwb eng 530 VZ Khriplovich, I. B. verfasserin aut Nonthermal radiation from black holes 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2002 Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. Radiation Black Hole Elementary Particle Particle Production Charged Black Hole Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 65(2002), 7 vom: Juli, Seite 1259-1270 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:65 year:2002 number:7 month:07 pages:1259-1270 https://doi.org/10.1134/1.1495025 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2279 AR 65 2002 7 07 1259-1270 |
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10.1134/1.1495025 doi (DE-627)OLC2049894368 (DE-He213)1.1495025-p DE-627 ger DE-627 rakwb eng 530 VZ Khriplovich, I. B. verfasserin aut Nonthermal radiation from black holes 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2002 Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. Radiation Black Hole Elementary Particle Particle Production Charged Black Hole Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 65(2002), 7 vom: Juli, Seite 1259-1270 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:65 year:2002 number:7 month:07 pages:1259-1270 https://doi.org/10.1134/1.1495025 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2279 AR 65 2002 7 07 1259-1270 |
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Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. © MAIK "Nauka/Interperiodica" 2002 |
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Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. © MAIK "Nauka/Interperiodica" 2002 |
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Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well. © MAIK "Nauka/Interperiodica" 2002 |
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B.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Nonthermal radiation from black holes</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2002</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">© MAIK "Nauka/Interperiodica" 2002</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract We consider particle production by charged and rotating black holes. A simple derivation is presented for the leading term (n=1) in the Schwinger formula for pair creation by a constant electric field. The same approach is then applied to charged-particle production by a charged black hole. The effect is due to the tunneling of created particles through an effective Dirac gap. Nonthermal radiation from a rotating black hole can also be explained in an analogous way. In the leading semiclassical approximation, this approach is applicable to bosons as well.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radiation</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Black Hole</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Elementary Particle</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Particle Production</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Charged Black Hole</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">Nauka/Interperiodica, 1993</subfield><subfield code="g">65(2002), 7 vom: Juli, Seite 1259-1270</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:65</subfield><subfield code="g">year:2002</subfield><subfield code="g">number:7</subfield><subfield code="g">month:07</subfield><subfield code="g">pages:1259-1270</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1134/1.1495025</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_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2004</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">65</subfield><subfield code="j">2002</subfield><subfield code="e">7</subfield><subfield code="c">07</subfield><subfield code="h">1259-1270</subfield></datafield></record></collection>
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