Titlebook: Quantum Mechanics in Curved Space-Time; Jürgen Audretsch,Venzo Sabbata Book 1990 Springer Science+Business Media New York 1990 Gravity.fie

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Vacuum States in Spacetimes with Killing Horizonshich is a thermal state for a static observer. Similarly, for de Sitter spacetime, Gibbons and Hawking (1977) defined the “Euclidean vacuum state” and showed that it has thermal properties for any inertial (geodesic) observer.

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The Final State of an Evaporating Black Hole and the Dimensionality of the Space-Timey the strong, weak and electromagnetic interactions. In recent times unification of electromagnetic and weak interactions has been reached through gauge theories and one can try to include also strong interactions.

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植物學(xué)

Quantum Strings in Curved Space Timeswe treat the case of boosted black-holes in the ultra relativist limit (gravitational schock wave or Aichelburg Sexl geometry) in the context of (i) the particle scattering at the Planck energy scale and (ii) quantum string dynamics and scattering in this geometry, (in this case, the problem can be solved exactly).

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