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- Hawking_radiation abstract "Hawking radiation is black body radiation that is predicted to be released by black holes, due to quantum effects near the event horizon.It is named after the physicist Stephen Hawking, who provided a theoretical argument for its existence in 1974, and sometimes also after Jacob Bekenstein, who predicted that black holes should have a finite, non-zero temperature and entropy.Hawking's work followed his visit to Moscow in 1973 where the Soviet scientists Yakov Zeldovich and Alexei Starobinsky showed him that according to the quantum mechanical uncertainty principle, rotating black holes should create and emit particles. Hawking radiation reduces the mass and the energy of the black hole and is therefore also known as black hole evaporation. Because of this, black holes that lose more mass than they gain through other means are expected to shrink and ultimately vanish. Micro black holes (MBHs) are predicted to be larger net emitters of radiation than larger black holes and should shrink and dissipate faster.In September 2010, a signal that is closely related to black hole Hawking radiation (see analog gravity) was claimed to have been observed in a laboratory experiment involving optical light pulses. However, the results remain unverified and debatable. Other projects have been launched to look for this radiation within the framework of analog gravity. In June 2008, NASA launched the Fermi space telescope, which will search for the terminal gamma-ray flashes expected from evaporating primordial black holes. In the event that speculative large extra dimension theories are correct, CERN's Large Hadron Collider may be able to create micro black holes and observe their evaporation.".
- Hawking_radiation thumbnail BH_LMC.png?width=300.
- Hawking_radiation wikiPageExternalLink 0212108,.
- Hawking_radiation wikiPageExternalLink 0503052,.
- Hawking_radiation wikiPageExternalLink 0602188.
- Hawking_radiation wikiPageExternalLink 0607081.
- Hawking_radiation wikiPageExternalLink hawk.html.
- Hawking_radiation wikiPageExternalLink Focus%20on%20Classical%20and%20Quantum%20Analogues%20for%20Gravitational%20Phenomena%20and%20Related%20Effects.
- Hawking_radiation wikiPageExternalLink Hawking-Radiation-Claimed-Created-In-a-Lab.
- Hawking_radiation wikiPageExternalLink 22.
- Hawking_radiation wikiPageExternalLink 317.
- Hawking_radiation wikiPageExternalLink vol59no11p44_48.pdf.
- Hawking_radiation wikiPageExternalLink hawking.
- Hawking_radiation wikiPageExternalLink theme3.py?level=1&index1=448732.
- Hawking_radiation wikiPageExternalLink 0607081.
- Hawking_radiation wikiPageID "173724".
- Hawking_radiation wikiPageRevisionID "603002944".
- Hawking_radiation hasPhotoCollection Hawking_radiation.
- Hawking_radiation subject Category:Astronomical_hypotheses.
- Hawking_radiation subject Category:Black_holes.
- Hawking_radiation subject Category:Quantum_field_theory.
- Hawking_radiation subject Category:Stephen_Hawking.
- Hawking_radiation type BlackHole109223177.
- Hawking_radiation type BlackHoles.
- Hawking_radiation type Location100027167.
- Hawking_radiation type Object100002684.
- Hawking_radiation type PhysicalEntity100001930.
- Hawking_radiation type Region108630039.
- Hawking_radiation type YagoGeoEntity.
- Hawking_radiation type YagoLegalActorGeo.
- Hawking_radiation type YagoPermanentlyLocatedEntity.
- Hawking_radiation comment "Hawking radiation is black body radiation that is predicted to be released by black holes, due to quantum effects near the event horizon.It is named after the physicist Stephen Hawking, who provided a theoretical argument for its existence in 1974, and sometimes also after Jacob Bekenstein, who predicted that black holes should have a finite, non-zero temperature and entropy.Hawking's work followed his visit to Moscow in 1973 where the Soviet scientists Yakov Zeldovich and Alexei Starobinsky showed him that according to the quantum mechanical uncertainty principle, rotating black holes should create and emit particles. ".
- Hawking_radiation label "Hawking radiation".
- Hawking_radiation label "Hawking-Strahlung".
- Hawking_radiation label "Hawkingstraling".
- Hawking_radiation label "Promieniowanie Hawkinga".
- Hawking_radiation label "Radiación de Hawking".
- Hawking_radiation label "Radiazione di Hawking".
- Hawking_radiation label "Radiação Hawking".
- Hawking_radiation label "Évaporation des trous noirs".
- Hawking_radiation label "Излучение Хокинга".
- Hawking_radiation label "إشعاع هوكينغ".
- Hawking_radiation label "ホーキング放射".
- Hawking_radiation label "霍金輻射".
- Hawking_radiation sameAs Hawkingovo_záření.
- Hawking_radiation sameAs Hawking-Strahlung.
- Hawking_radiation sameAs Radiación_de_Hawking.
- Hawking_radiation sameAs Évaporation_des_trous_noirs.
- Hawking_radiation sameAs Radiasi_Hawking.
- Hawking_radiation sameAs Radiazione_di_Hawking.
- Hawking_radiation sameAs ホーキング放射.
- Hawking_radiation sameAs 호킹_복사.
- Hawking_radiation sameAs Hawkingstraling.
- Hawking_radiation sameAs Promieniowanie_Hawkinga.
- Hawking_radiation sameAs Radiação_Hawking.
- Hawking_radiation sameAs m.017fn5.
- Hawking_radiation sameAs Q497396.
- Hawking_radiation sameAs Q497396.
- Hawking_radiation sameAs Hawking_radiation.
- Hawking_radiation wasDerivedFrom Hawking_radiation?oldid=603002944.
- Hawking_radiation depiction BH_LMC.png.
- Hawking_radiation isPrimaryTopicOf Hawking_radiation.
