Testing continuous spontaneous localization with Fermi liquids
Testing continuous spontaneous localization with Fermi liquids
Collapse models describe phenomenologically the quantum-to-classical transition by adding suitable nonlinear and stochastic terms to the Schrödinger equation, thus (slightly) modifying the dynamics of quantum systems. Experimental bounds on the collapse parameters have been derived from various experiments involving a plethora of different systems, from single atoms to gravitational wave detectors. Here, we give a comprehensive treatment of the continuous spontaneous localization (CSL) model, the most studied among collapse models, for Fermi liquids. We consider both the white and non-white noise case. Application to various astrophysical sources is presented.
1-7
Adler, Stephen L.
59ee296f-da05-496a-a9e7-4b043900e8ac
Bassi, Angelo
374a70f7-61f8-4656-bb45-5857695750f1
Carlesso, Matteo
bdaf218c-85ae-43fb-a347-47800841078e
Vinante, Andrea
f023d600-0537-41c4-b307-bf9cdfc1f56c
15 May 2019
Adler, Stephen L.
59ee296f-da05-496a-a9e7-4b043900e8ac
Bassi, Angelo
374a70f7-61f8-4656-bb45-5857695750f1
Carlesso, Matteo
bdaf218c-85ae-43fb-a347-47800841078e
Vinante, Andrea
f023d600-0537-41c4-b307-bf9cdfc1f56c
Adler, Stephen L., Bassi, Angelo, Carlesso, Matteo and Vinante, Andrea
(2019)
Testing continuous spontaneous localization with Fermi liquids.
Physical Review D, 99 (10), , [103001].
(doi:10.1103/PhysRevD.99.103001).
Abstract
Collapse models describe phenomenologically the quantum-to-classical transition by adding suitable nonlinear and stochastic terms to the Schrödinger equation, thus (slightly) modifying the dynamics of quantum systems. Experimental bounds on the collapse parameters have been derived from various experiments involving a plethora of different systems, from single atoms to gravitational wave detectors. Here, we give a comprehensive treatment of the continuous spontaneous localization (CSL) model, the most studied among collapse models, for Fermi liquids. We consider both the white and non-white noise case. Application to various astrophysical sources is presented.
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e-pub ahead of print date: 10 May 2019
Published date: 15 May 2019
Identifiers
Local EPrints ID: 430965
URI: http://eprints.soton.ac.uk/id/eprint/430965
ISSN: 2470-0029
PURE UUID: d1452917-f6d1-40a4-a229-785e017c7ed7
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Date deposited: 20 May 2019 16:30
Last modified: 16 Mar 2024 01:51
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Contributors
Author:
Stephen L. Adler
Author:
Angelo Bassi
Author:
Matteo Carlesso
Author:
Andrea Vinante
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