Amplification of the black-hole Hawking radiation by stimulated emission
If bosonic particles or antiparticles are sent in during the collapse to a Schwarzschild black hole, they stimulate an additional creation of particle-antiparticle pairs out of the curved background. This results in an induced amplification of the thermal Hawking radiation. Using wave-packet modes,...
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| Veröffentlicht in: | Physical review. D, Particles and fields Particles and fields, 1992-01, Vol.45 (2), p.513-519 |
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| container_title | Physical review. D, Particles and fields |
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| creator | AUDRETSCH, J MÜLLER, R |
| description | If bosonic particles or antiparticles are sent in during the collapse to a Schwarzschild black hole, they stimulate an additional creation of particle-antiparticle pairs out of the curved background. This results in an induced amplification of the thermal Hawking radiation. Using wave-packet modes, we show that the packet of incoming particles reappears in the out region at a time and with an energy which corresponds to the propagation and redshift of classical ray optics. It is accompanied by additional particles of the same energy. Their intensity varies with energy according to the thermal Hawking spectrum and is proportional to the number of incoming particles. Another contribution of the same structure goes back to antiparticles coming in at a different trajectory. They stimulate the emission of additional pairs. The respective antiparticles fall through the horizon and their particle partners add to the outgoing-particle content. A localization of the processes is obtained. |
| doi_str_mv | 10.1103/physrevd.45.513 |
| format | Article |
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This results in an induced amplification of the thermal Hawking radiation. Using wave-packet modes, we show that the packet of incoming particles reappears in the out region at a time and with an energy which corresponds to the propagation and redshift of classical ray optics. It is accompanied by additional particles of the same energy. Their intensity varies with energy according to the thermal Hawking spectrum and is proportional to the number of incoming particles. Another contribution of the same structure goes back to antiparticles coming in at a different trajectory. They stimulate the emission of additional pairs. The respective antiparticles fall through the horizon and their particle partners add to the outgoing-particle content. 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D, Particles and fields</title><addtitle>Phys Rev D Part Fields</addtitle><description>If bosonic particles or antiparticles are sent in during the collapse to a Schwarzschild black hole, they stimulate an additional creation of particle-antiparticle pairs out of the curved background. This results in an induced amplification of the thermal Hawking radiation. Using wave-packet modes, we show that the packet of incoming particles reappears in the out region at a time and with an energy which corresponds to the propagation and redshift of classical ray optics. It is accompanied by additional particles of the same energy. Their intensity varies with energy according to the thermal Hawking spectrum and is proportional to the number of incoming particles. Another contribution of the same structure goes back to antiparticles coming in at a different trajectory. They stimulate the emission of additional pairs. 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D, Particles and fields</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>AUDRETSCH, J</au><au>MÜLLER, R</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Amplification of the black-hole Hawking radiation by stimulated emission</atitle><jtitle>Physical review. D, Particles and fields</jtitle><addtitle>Phys Rev D Part Fields</addtitle><date>1992-01-15</date><risdate>1992</risdate><volume>45</volume><issue>2</issue><spage>513</spage><epage>519</epage><pages>513-519</pages><issn>0556-2821</issn><eissn>1089-4918</eissn><coden>PRVDAQ</coden><abstract>If bosonic particles or antiparticles are sent in during the collapse to a Schwarzschild black hole, they stimulate an additional creation of particle-antiparticle pairs out of the curved background. This results in an induced amplification of the thermal Hawking radiation. Using wave-packet modes, we show that the packet of incoming particles reappears in the out region at a time and with an energy which corresponds to the propagation and redshift of classical ray optics. It is accompanied by additional particles of the same energy. Their intensity varies with energy according to the thermal Hawking spectrum and is proportional to the number of incoming particles. Another contribution of the same structure goes back to antiparticles coming in at a different trajectory. They stimulate the emission of additional pairs. The respective antiparticles fall through the horizon and their particle partners add to the outgoing-particle content. A localization of the processes is obtained.</abstract><cop>Ridge, NY</cop><pub>American Physical Society</pub><pmid>10014403</pmid><doi>10.1103/physrevd.45.513</doi><tpages>7</tpages></addata></record> |
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| ispartof | Physical review. D, Particles and fields, 1992-01, Vol.45 (2), p.513-519 |
| issn | 0556-2821 1089-4918 |
| language | eng |
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| source | American Physical Society Journals |
| subjects | 662440 -- Properties of Other Particles Including Hypothetical Particles-- (1992-) ANTIMATTER ANTIPARTICLES BLACK HOLES BOSONS DIFFERENTIAL EQUATIONS ELECTROMAGNETIC RADIATION ELEMENTARY PARTICLES EMISSION ENERGY SPECTRA ENERGY-LEVEL TRANSITIONS EQUATIONS Exact sciences and technology FIELD THEORIES General relativity and gravitation GRAVITATIONAL COLLAPSE INTERACTIONS KLEIN-GORDON EQUATION MATRICES MATTER PAIR PRODUCTION PARTIAL DIFFERENTIAL EQUATIONS PARTICLE PRODUCTION Physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS PROBABILITY QUANTUM FIELD THEORY Quantum gravity RADIATIONS RED SHIFT S MATRIX SCALAR FIELDS SCHWARZSCHILD RADIUS SPECTRA STIMULATED EMISSION THERMAL RADIATION UNIVERSE WAVE EQUATIONS 662110 -- General Theory of Particles & Fields-- Theory of Fields & Strings-- (1992-) |
| title | Amplification of the black-hole Hawking radiation by stimulated emission |
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