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  1. Energy-momentum tensor near an evaporating black hole.P. C. W. Davies & S. A. Fulling - unknown
    two dimensions, quantum radiation production is incompatible with a conserved and traceless T„,. We therefore resolve an ambiguity in our expression for Tr„, regularized by a geodesic point-separation procedure.
     
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  2.  17
    Physical States and Renormalized Observables in Quantum Field Theories with External Gravity.S. A. Fulling - 1980 - In A. R. Marlow (ed.), Quantum theory and gravitation. New York: Academic Press. pp. 1--187.
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  3.  15
    2 V ds= guvdxudx.S. A. Fulling - 1980 - In A. R. Marlow (ed.), Quantum theory and gravitation. New York: Academic Press. pp. 187.
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  4. Interacting Bosons at Finite Temperature: How Bogolubov Visited a Black Hole and Came Home Again. [REVIEW]S. A. Fulling, B.-G. Englert & M. D. Pilloff - 2003 - Foundations of Physics 33 (1):87-110.
    The structure of the thermal equilibrium state of a weakly interacting Bose gas is of current interest. We calculate the density matrix of that state in two ways. The most effective method, in terms of yielding a simple, explicit answer, is to construct a generating function within the traditional framework of quantum statistical mechanics. The alternative method, arguably more interesting, is to construct the thermal state as a vector state in an artificial system with twice as many degrees of freedom. (...)
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