GGTCAAGGGGCCAATAGAGAGGCTCCTCTCTCACTCGCTAGGAGGCAATTGTATAACAATGCTTACTGCATCGATACATAAAACGTGTCCATCGGTTGCCCAAACTGTGAAGTGTCTATCACCCCTAGGCCCGTTTCCCGCATATAAACGCCAGGTTGTATCCGCATTTGATGCTACCGTGGATGAGTCAGCGTCGAGCACGCGGCA
GGAGTGAGCCTACCTCCGTTTGCGTCTTGTTACCAATGAAAAAGCTATGCACTTTGTACAGGGTGCCATCGGGTTTCTGAACTCTCAGATAGTGGGGATCCCGGGAAAGGGCCTATATTTGCGGTCCAACTTAGGCGTAAACCTCGATGCTACCTACTCAGACCCACCCCGCGCGGGGTAAATATGGCACTCATCCCAGCTGGTTC
TCAAGGTTACTTTTTGGATACCTGAAACAAATCCCATGGTAGTCCTTAGACTTGGGAGTCTATCACCCCTAGGGCCCATATCTGGAAATAGACGCCAAGTTCAATCCGTATTCCGACGTACGATGGAACAGTGTGGGTGAGACGTGCTTCATTTATACCCTACGCAGGCTGGACCGAGGTCCGCAAGGCGCGGCGGTGCACAAGCAA
test post gallery

A star collapsing gravitationally into a black hole emits a flux of radiation, knowns as Hawking radiation. When the initial state of a quantum field on the background of the star, is placed in the Unruh vacuum in the far past, then Hawking radiation corresponds to a flux of positive energy radiation travelling outwards to future infinity.

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