quantum field theory in curved spacetime

See Quantum field theory in curved spacetime for a more complete discussion.

During the late 1960s, Parker established a new area of physics - quantum field theory in curved spacetime.

More recently, the approach has been further implemented to include an algebraic version of quantum field theory in curved spacetime.

Also quantum field theory in curved spacetime).

The theory of quantum field theory in curved spacetime can be considered as a first approximation to quantum gravity.

Quantum field theory in curved spacetime predicts that event horizons emit radiation like a black body with a finite temperature.

Davies' inquiries have included theoretical physics, cosmology, and astrobiology; his research has been mainly in the area of quantum field theory in curved spacetime.

In quantum field theory in curved spacetime, there is a unique quantum state over a background de Sitter space which is invariant under all the isometries.

In particle physics, quantum field theory in curved spacetime is an extension of standard, Minkowski-space quantum field theory to curved spacetime.

It is possible to formulate quantum field theory in curved spacetime, yet even this still cannot incorporate GR because gravity is not renormalizable in QFT.

In order to describe situations in which gravity is strong enough to influence (quantum) matter, yet not strong enough to require quantization itself, physicists have formulated quantum field theories in curved spacetime.

It is yet unknown how gravity can be incorporated into quantum mechanics, nevertheless, far from the black hole the gravitational effects can be weak enough for calculations to be reliably performed in the framework of quantum field theory in curved spacetime.