Semiclassical Wheeler wormhole production
It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1991 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
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| Übergeordnetes Werk: |
in: Physics Letters B - Amsterdam : Elsevier, 256(1991), 2, Seite 146-149 |
| Übergeordnetes Werk: |
volume:256 ; year:1991 ; number:2 ; pages:146-149 |
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| 520 | |a It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. | ||
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(DE-627)NLEJ181583100 (DE-599)GBVNLZ181583100 DE-627 ger DE-627 rakwb eng Semiclassical Wheeler wormhole production 1991 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Garfinkle, D. oth Strominger, A. oth in Physics Letters B Amsterdam : Elsevier 256(1991), 2, Seite 146-149 (DE-627)NLEJ177212217 (DE-600)1466612-1 0370-2693 nnns volume:256 year:1991 number:2 pages:146-149 http://linkinghub.elsevier.com/retrieve/pii/0370-2693(91)90665-D GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 256 1991 2 146-149 |
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(DE-627)NLEJ181583100 (DE-599)GBVNLZ181583100 DE-627 ger DE-627 rakwb eng Semiclassical Wheeler wormhole production 1991 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Garfinkle, D. oth Strominger, A. oth in Physics Letters B Amsterdam : Elsevier 256(1991), 2, Seite 146-149 (DE-627)NLEJ177212217 (DE-600)1466612-1 0370-2693 nnns volume:256 year:1991 number:2 pages:146-149 http://linkinghub.elsevier.com/retrieve/pii/0370-2693(91)90665-D GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 256 1991 2 146-149 |
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(DE-627)NLEJ181583100 (DE-599)GBVNLZ181583100 DE-627 ger DE-627 rakwb eng Semiclassical Wheeler wormhole production 1991 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Garfinkle, D. oth Strominger, A. oth in Physics Letters B Amsterdam : Elsevier 256(1991), 2, Seite 146-149 (DE-627)NLEJ177212217 (DE-600)1466612-1 0370-2693 nnns volume:256 year:1991 number:2 pages:146-149 http://linkinghub.elsevier.com/retrieve/pii/0370-2693(91)90665-D GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 256 1991 2 146-149 |
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(DE-627)NLEJ181583100 (DE-599)GBVNLZ181583100 DE-627 ger DE-627 rakwb eng Semiclassical Wheeler wormhole production 1991 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Garfinkle, D. oth Strominger, A. oth in Physics Letters B Amsterdam : Elsevier 256(1991), 2, Seite 146-149 (DE-627)NLEJ177212217 (DE-600)1466612-1 0370-2693 nnns volume:256 year:1991 number:2 pages:146-149 http://linkinghub.elsevier.com/retrieve/pii/0370-2693(91)90665-D GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 256 1991 2 146-149 |
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(DE-627)NLEJ181583100 (DE-599)GBVNLZ181583100 DE-627 ger DE-627 rakwb eng Semiclassical Wheeler wormhole production 1991 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Garfinkle, D. oth Strominger, A. oth in Physics Letters B Amsterdam : Elsevier 256(1991), 2, Seite 146-149 (DE-627)NLEJ177212217 (DE-600)1466612-1 0370-2693 nnns volume:256 year:1991 number:2 pages:146-149 http://linkinghub.elsevier.com/retrieve/pii/0370-2693(91)90665-D GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 256 1991 2 146-149 |
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Semiclassical Wheeler wormhole production |
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It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. |
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It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. |
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It is argued that if topology change is allowed in quantum gravity, it is possible to create a Wheeler wormhole, i.e. a pair of oppositely charged extreme Reissner-Nordstrom black holes identified at their throats, in an electromagnetic field. The instanton describing this process is found, and the tunneling rate computed in the semiclassical approximation. |
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