An effective model for the spacetime foam is constructed in terms of nonlocal interactions in a classical background. In the weak coupling approximation, the evolution of the low-energy density matrix is determined by a master equation that predicts loss of quantum coherence. Moreover, spacetime foam can be described by a quantum thermal field that, apart from inducing loss of coherence, gives rise to effects such as gravitational Lamb and Stark shifts as well as quantum damping in the evolution of the low-energy observables.
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Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy
Ist Nazl Fis Nucl, Sez Roma 1, Ple A Moro 2, I-00185 Rome, ItalyUniv Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy
Amelino-Camelia, Giovanni
Brighenti, Francesco
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Imperial Coll, Blackett Lab, Theoret Phys, London SW7 2BZ, England
Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, ItalyUniv Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy
Brighenti, Francesco
Gubitosi, Giulia
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Imperial Coll, Blackett Lab, Theoret Phys, London SW7 2BZ, EnglandUniv Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy
Gubitosi, Giulia
Santos, Grasiele
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机构:Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy