Abstract
Quantum field theory on curved spacetime is a generalisation of quantum field theory in flat spacetime which is expected to be the proper fundamental description of non–trivial physical phenomena in the presence of a spacetime curvature which is large but below Planck scale. Two prominent physical situations which fall under this characterisation are phenomena both in the vicinity of black holes and in the early universe. Focusing on the latter, we review several applications of algebraic quantum field theory on curved spacetimes to cosmology, as well as foundational results and constructions on which these applications are based. On the foundational side, we collect several proposals to construct Hadamard states on cosmological spacetimes, as this class of states is believed to encompass all physically meaningful states in quantum field theory on curved spacetimes. Afterwards we consider the solution theory of the semiclassical Einstein equation, quote a theorem of existence and uniqueness of solutions to this equation and indicate directions to go beyond the semiclassical Einstein equation. Then we highlight how the observed cosmological expansion may be understood qualitatively and quantitatively in this framework, before we discuss the quantization of perturbations in inflation in the context of algebraic quantum field theory. In the latter subject, the starting point is the assumption that the classical, rather than the semiclassical, Einstein equation is satisfied. We close this chapter briefly discussing how one may generalise the analysis of perturbations in inflation by allowing for spacetimes backgrounds which solve the semiclassical Einstein equations.
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Strictly speaking \({\mathcal {L}}_\varsigma EL({\mathfrak {G}})=0\) is satisfied even if \(\Box \varphi + \partial _\varphi V=c\) with c constant but non–zero. However, one may absorb c by redefining \(V(\varphi )\).
References
Ade, P.A.R., et al.: [Planck Collaboration]: Planck 2013 results. XVI. Cosmological parameters. Astron. Astrophys. 571, A16 (2014)
Ade, P.A.R., et al.: [Planck Collaboration]: Planck 2013 results. XXII. Constraints on inflation. Astron. Astrophys. 571, A22 (2014)
Ade, P.A.R., et al.: [BICEP2 Collaboration]: Detection of B-Mode polarization at degree angular scales by BICEP2. Phys. Rev. Lett. 112, 241101 (2014)
Afshordi, N., Aslanbeigi, S., Sorkin, R.D.: A distinguished vacuum state for a quantum field in curved spacetime: formalism, features, and cosmology. JHEP 2012, 1–12 (2012)
Anderson, P.R.: Effects of quantum fields on singularities and particle horizons in the early universe. 4. initially empty universes. Phys. Rev. D 33, 1567 (1986)
Brum, M., Fredenhagen, K.: ‘Vacuum-like’ Hadamard states for quantum fields on curved spacetimes. Class. Quantum Grav. 31, 025024 (2014)
Brunetti, R., Fredenhagen, K., Hollands, S.: A remark on alpha vacua for quantum field theories on de Sitter space. JHEP 0505, 063 (2005)
Brunetti, R., Fredenhagen, K., Köhler, M.: The microlocal spectrum condition and wick polynomials of free fields on curved spacetimes. Commun. Math. Phys. 180, 633–652 (1996)
Brunetti, R., Fredenhagen, K., Verch, R.: The generally covariant locality principle—a new paradigm for local quantum field theory. Commun. Math. Phys. 237, 31–68 (2003)
Dappiaggi, C., Hack, T.-P., Pinamonti, N.: Approximate KMS states for scalar and spinor fields in Friedmann-Robertson-Walker spacetimes. Ann. Henri Poincare 12, 1449 (2011)
Dappiaggi, C., Moretti, V., Pinamonti, N.: Cosmological horizons and reconstruction of quantum field theories. Commun. Math. Phys. 285, 1129–1163 (2009)
Dappiaggi, C., Moretti, V., Pinamonti, N.: Distinguished quantum states in a class of cosmological spacetimes and their Hadamard property. J. Math. Phys. 50, 062304 (2009)
Dimock, J.: Quantized electromagnetic field on a manifold. Rev. Math. Phys. 4, 223–233 (1992)
Degner, A.: Properties of states of low energy on cosmological spacetimes. PhD thesis, University of Hamburg (2013)
Eltzner, B.: Quantization of perturbations in Inflation. arXiv:1302.5358 [gr-qc]
Eltzner, B., Gottschalk, H.: Dynamical backreaction in Robertson-Walker spacetime. Rev. Math. Phys. 23, 531–551 (2011)
Fewster, C.J., Hunt, D.S.: Quantization of linearised gravity in cosmological vacuum spacetimes. Rev. Math. Phys. 25, 1330003 (2013)
Fewster, C.J., Verch, R.: On a recent construction of ‘Vacuum-like’ quantum field states in curved spacetime. Class. Quant. Grav. 29, 205017 (2012)
Fewster, C.J., Ford, L.H., Roman, T.A.: Probability distributions of smeared quantum stress tensors. Phys. Rev. D 81, 121901 (2010)
Gérard, C., Wrochna, M.: Construction of Hadamard states by pseudo-differential calculus. Comm. Math. Phys. 325, 713–755 (2014)
Hack, T.-P.: The Lambda CDM-model in quantum field theory on curved spacetime and dark radiation. arXiv:1306.3074 [gr-qc]
Hack, T.-P.: Quantization of the linearised Einstein-Klein-Gordon system on arbitrary backgrounds and the special case of perturbations in Inflation. Class. Quantum Grav. 31, 215004 (2014)
Hack, T.-P., Schenkel, A.: Linear bosonic and fermionic quantum gauge theories on curved spacetimes. Gen. Rel. Grav. 45, 877 (2013)
Hollands, S., Wald, R.M.: Local wick polynomials and time ordered products of quantum fields in curved spacetime. Commun. Math. Phys. 223, 289–326 (2001)
Hollands, S., Wald, R.M.: Existence of local covariant time ordered products of quantum fields in curved spacetime. Commun. Math. Phys. 231, 2309 (2002)
Hollands, S., Wald, R.M.: Conservation of the stress tensor in interacting quantum field theory in curved spacetimes. Rev. Math. Phys. 17, 227 (2005)
Hu, B.L., Verdaguer, E.: Stochastic gravity: theory and applications. Living Rev. Rel. 11, 3 (2008); Living Rev. Rel. 7, 3 (2004)
Junker, W., Schrohe, E.: Adiabatic vacuum states on general spacetime manifolds: definition, construction, and physical properties. Ann. Henri Poincaré 3, 1113–1181 (2002)
Kay, B.S., Wald, R.M.: Theorems on the uniqueness and thermal properties of stationary, nonsingular, Quasifree states on space-times with a bifurcate killing horizon. Phys. Rept. 207, 49 (1991)
Kolb, E.W., Turner, M.S.: The early universe. Front. Phys. 69, 1 (1990)
Küskü, M.: A class of almost equilibrium states in Robertson-Walker spacetimes. DESY-THESIS-2008-020
Lüders, C., Roberts, J.E.: Local quasiequivalence and adiabatic vacuum states. Commun. Math. Phys. 134, 29–63 (1990)
Moretti, V.: Comments on the stress-energy tensor operator in curved spacetime. Commun. Math. Phys. 232, 189–221 (2003)
Olbermann, H.: States of low energy on Robertson-Walker spacetimes. Class. Quantum Grav. 24, 5011–5030 (2007)
Parker, L.: Quantized fields and particle creation in expanding universes I. Phys. Rev. 183, 1057–1068 (1969)
Pinamonti, N.: On the initial conditions and solutions of the semiclassical Einstein equations in a cosmological scenario. Commun. Math. Phys. 305, 563–604 (2011)
Pinamonti, N., Siemssen, D.: Scale-invariant curvature fluctuations from an extended semiclassical gravity. J. Math. Phys. 56, 022303 (2015)
Pinamonti, N., Siemssen, D.: Global existence of solutions of the semiclassical Einstein equation for cosmological spacetimes. Commun. Math. Phys. 334(1), 171–191 (2015)
Radzikowski, M.J.: Micro-local approach to the hadamard condition in quantum field theory on curved space-time. Commun. Math. Phys. 179, 529–553 (1996)
Riegert, R.J.: A nonlocal action for the trace anomaly. Phys. Lett. B 134, 56 (1984)
Schlemmer, J.: Ph.D. thesis, Faculty of Physics, University of Leipzig (2010)
Sewell, G. L.: Quantum fields on manifolds: PCT and gravitationally induced thermal states, Ann. Phys. (NY) 141, 201 (1982)
Straumann, N.: From primordial quantum fluctuations to the anisotropies of the cosmic microwave background radiation. Annalen Phys. 15, 70 (2006)
Starobinsky, A.A.: A new type of isotropic cosmological models without singularity. Phys. Lett. B 91, 99 (1980)
Starobinsky, A.A.: The perturbation spectrum evolving from a nonsingular initially de-sitter cosmology and the microwave background anisotropy. Sov. Astron. Lett. 9, 302 (1983)
Them, K., Brum, M.: States of low energy in homogeneous and inhomogeneous. Expanding Spacetimes. Class. Quant. Grav. 30, 235035 (2013)
Verch, R.: Local covariance, renormalization ambiguity, and local thermal equilibrium in cosmology. In: Finster, F., Müller, O., Nardmann, M., Tolksdorf, J., Zeidler, E. (eds.) Quantum field theory and gravity. Conceptual and mathematical advances in the search for a unified framework, Birkhäuser (2012)
Wald, R.M.: Axiomatic renormalization of stress tensor of a conformally invariant field in conformally flat spacetimes. Ann. Phys. 110, 472 (1978)
Wald, R.M.: Trace anomaly of a conformally invariant quantum field in curved space-time. Phys. Rev. D 17, 1477 (1978)
Zschoche, J.: The Chaplygin gas equation of state for the quantized free scalar field on cosmological spacetimes. Ann. Henri Poincare 15, 1285 (2014)
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Hack, TP., Pinamonti, N. (2015). Cosmological Applications of Algebraic Quantum Field Theory. In: Brunetti, R., Dappiaggi, C., Fredenhagen, K., Yngvason, J. (eds) Advances in Algebraic Quantum Field Theory. Mathematical Physics Studies. Springer, Cham. https://doi.org/10.1007/978-3-319-21353-8_6
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