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General Relativity Consider a spherical blackbody of constant temperature and mass M whose surface lies at radial coordinate r =R. An observer located at the surface of the sphere and a distant observer both measure the blackbody radiation given off by the sphere.Both observers use Wien's law,the below equation, to determine the blackbody's temperature. Show that 2GM T = T1- Rc² *

General Relativity Consider a spherical blackbody of constant temperature and mass M whose surface lies at radial coordinate r =R. An observer located at the surface of the sphere and a distant observer both measure the blackbody radiation given off by the sphere.Both observers use Wien's law,the below equation, to determine the blackbody's temperature. Show that 2GM T = T1- Rc² *

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General Relativity Consider a spherical blackbody of constant temperature and mass M whose surface lies at radial coordinate r = R. An observer located at the surface of the sphere and a distant observer both measure the blackbody radiation given off by the sphere.Both observers use Wien's law, the below equation, to determine the blackbody's temperature. Show that 2GM T = T/1 Rc2
Transcribed Image Text:General Relativity Consider a spherical blackbody of constant temperature and mass M whose surface lies at radial coordinate r = R. An observer located at the surface of the sphere and a distant observer both measure the blackbody radiation given off by the sphere.Both observers use Wien's law, the below equation, to determine the blackbody's temperature. Show that 2GM T = T/1 Rc2
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