For a quantum field living on a nonstatic space–time no instantaneous Hamiltonian is definable, for this generically necessitates a choice of inequivalent representation of the canonical commutation relations at each instant of time. This fact suggests a description in terms of time-dependent Hilbert spaces, a concept that fits naturally in a (consistent) histories framework. Our primary tool for the construction of the quantum theory in a continuous-time histories format is the recently developed formalism based on the notion of the history group. This we employ to study a model system involving a 1+1 scalar field in a cavity with moving boundaries. The instantaneous (smeared) Hamiltonian and a decoherence functional are then rigorously defined so that finite values for the time-averaged particle creation rate are obtainable through the study of energy histories. We also construct the Schwinger–Keldysh closed-time-path generating functional as a “Fourier transform” of the decoherence functional and evaluate the corresponding n-point functions.

1.
R. B.
Griffiths
, “
Consistent histories and the interpretation of quantum mechanics
,”
J. Stat. Phys.
36
,
219
(
1984
).
2.
R.
Omnès
, “
Logical reformulation of quantum mechanics. I. Foundations
,”
J. Stat. Phys.
53
,
893
(
1988
);
The Interpretation of Quantum Mechanics (Princeton University Press, Princeton, 1994).
3.
M.
Gell-Mann
and
J. B.
Hartle
, Quantum Mechanics in the Light of Quantum Cosmology, in Complexity, Entropy, and the Physics of Information, edited by W. Zurek (Addison–Wesley, Reading, 1990);
M.
Gell-Mann
and
J. B.
Hartle
, “
Classical equations for quantum systems
,”
Phys. Rev. D
47
,
3345
(
1993
).
4.
J. B. Hartle, “Space–time quantum mechanics and the quantum mechanics of space–time,” in Proceedings of the 1992 Les Houches School, Gravitation and Quantizations, 1993 (unpublished).
5.
C. J.
Isham
, “
Quantum logic and the histories approach to quantum theory
,”
J. Math. Phys.
35
,
2157
(
1994
);
C. J.
Isham
and
N.
Linden
, “
Quantum temporal logic and decoherence functionals in the histories approach to generalized quantum theory
,”
J. Math. Phys.
35
,
5472
(
1994
).
6.
C. J.
Isham
,
N.
Linden
, and
S.
Schreckenberg
, “
The classification of decoherence functionals: An analog of Gleason’s theorem
,”
J. Math. Phys.
35
,
6360
(
1994
).
7.
C. J. Isham, Topological and Global Aspects of Quantum Theory, in Relativity, Groups, and Topology II (Les Houches, 1983).
8.
C. J.
Isham
and
N.
Linden
, “
Continuous histories and the history group in generalized quantum theory
,”
J. Math. Phys.
36
,
5392
(
1995
).
9.
C. J.
Isham
,
N.
Linden
,
K.
Savvidou
, and
S.
Schreckenberg
, “
Continuous time and consistent histories
,”
J. Math. Phys.
39
,
1818
(
1998
).
10.
K.
Savvidou
, “
The action operator in continuous-time histories
,” gr-qc/9811078.
11.
J. S.
Schwinger
, “
Brownian motion of a quantum oscillator
,”
J. Math. Phys.
2
,
407
(
1961
);
L. V.
Keldysh
, “
Diagram technique for nonequilibrium processes
,”
Zh. Eksp. Teor. Fiz.
47
,
1515
(
1964
);
for a recent treatment, see
E.
Calzetta
and
B. L.
Hu
, “
Closed time path functional formalism in curved space–time: Application to cosmological backreaction problems
,”
Phys. Rev. D
35
,
495
(
1987
).
12.
A.
Ashtekar
and
A.
Magnon
, “
Quantum fields in curved space–times
,”
Proc. R. Soc. London, Ser. A
346
,
375
(
1975
).
13.
S.
Schreckenberg
, “
Symmetry and history quantum theory: An analog of Wigner’s theorem
,”
J. Math. Phys.
37
,
6086
(
1997
);
S.
Schreckenberg
, “
Symmetries of Decoherence Functionals
,”
J. Math. Phys.
38
,
759
(
1997
).
14.
F. A. Berezin, The Method of Second Quantization (Academic, New York, 1966).
15.
R. Wald, Quantum Field Theory in Curved Space–Time and Black Hole Thermodynamics (University of Chicago Press, Chicago, 1994).
16.
R. F. Streater and A. S. Wightman, PCT, Spin, Statistics, and All That (Benjamin, New York, 1964).
17.
N. B. Birrell and P. C. W. Davies, Quantum Fields in Curved Space (Cambridge University Press, Cambridge, 1982).
18.
S. Janson, Gaussian Hilbert Spaces (Cambridge University Press, Cambridge, 1997).
19.
J. R.
Klauder
, “
Quantization is geometry, after all
,”
Ann. Phys. (N.Y.)
188
,
120
(
1988
).
20.
R. D.
Sorkin
, “
Quantum mechanics as quantum measure theory
,”
Mod. Phys. Lett. A
9
,
3119
(
1994
);
Quantum Measure Theory and its Interpretation, in Quantum Classical Correspondence, edited by D. H. Feng and B. L. Hu (International Press, Cambridge, MA, 1997).
21.
C.
Anastopoulos
, “
Selection of preferred consistent sets
,”
Int. J. Theor. Phys.
37
,
2261
(
1998
).
22.
P. C. W.
Davies
and
S. A.
Fulling
, “
Radiation from moving mirrors and from black holes
,”
Proc. R. Soc. London
356
,
237
(
1977
).
23.
S. A.
Fulling
,
M.
Sweeny
, and
R. M.
Wald
, “
Singularity structure of the two-point function in quantum field theory in curved space–time
,”
Commun. Math. Phys.
63
,
257
(
1978
).
24.
I.
Kouletsis
, “
A classical history theory: Geometrodynamics and general field dynamics regained
,” gr-qc/9801019.
25.
E.
Calzetta
and
B. L.
Hu
, “
Noise and fluctuations in semiclassical gravity
,”
Phys. Rev. D
49
,
6636
(
1994
);
E.
Calzetta
,
A.
Campos
, and
E.
Verdaguer
, “
Stochastic semiclassical cosmological models
,”
Phys. Rev. D
56
,
2163
(
1997
);
R.
Martin
and
E.
Verdaguer
, “
An effective stochastic semiclassical theory for the gravitational field
,” gr-qc/9812063.
26.
J. B.
Hartle
, “
Generalized quantum theory and black hole evaporation
,” gr-qc/980870.
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