The University of Southampton
University of Southampton Institutional Repository

Testing spontaneous collapse through bulk heating experiments: An estimate of the background noise

Testing spontaneous collapse through bulk heating experiments: An estimate of the background noise
Testing spontaneous collapse through bulk heating experiments: An estimate of the background noise
Models of spontaneous wave function collapse predict a small heating rate for a bulk solid, as a result of coupling to the noise field that causes collapse. This rate is small enough that ambient radioactivity and cosmic ray flux on the surface of the earth can mask the heating due to spontaneous collapse. In this paper we estimate the background noise due to γ radiation and cosmic ray muon flux, at different depths. We demonstrate that a low-temperature underground experiment at a depth of about 6.5 kilometer water equivalent would have a low enough background to allow detection of bulk heating for a collapse rate λ of 10−16s−1 using presently available technology.
2469-9926
Mishra, Ruchira
8cbe036c-691d-4d3a-89eb-eafd44a22c86
Vinante, Andrea
f023d600-0537-41c4-b307-bf9cdfc1f56c
Singh, Tejinder
8770ddc2-08a8-47a6-bc59-40efca966a22
Mishra, Ruchira
8cbe036c-691d-4d3a-89eb-eafd44a22c86
Vinante, Andrea
f023d600-0537-41c4-b307-bf9cdfc1f56c
Singh, Tejinder
8770ddc2-08a8-47a6-bc59-40efca966a22

Mishra, Ruchira, Vinante, Andrea and Singh, Tejinder (2018) Testing spontaneous collapse through bulk heating experiments: An estimate of the background noise. Physical Review A, 98 (5), [052121]. (doi:10.1103/PhysRevA.98.052121).

Record type: Article

Abstract

Models of spontaneous wave function collapse predict a small heating rate for a bulk solid, as a result of coupling to the noise field that causes collapse. This rate is small enough that ambient radioactivity and cosmic ray flux on the surface of the earth can mask the heating due to spontaneous collapse. In this paper we estimate the background noise due to γ radiation and cosmic ray muon flux, at different depths. We demonstrate that a low-temperature underground experiment at a depth of about 6.5 kilometer water equivalent would have a low enough background to allow detection of bulk heating for a collapse rate λ of 10−16s−1 using presently available technology.

Text
bulkheatingnoise_last - Accepted Manuscript
Download (703kB)

More information

Accepted/In Press date: 23 October 2018
e-pub ahead of print date: 16 November 2018
Published date: November 2018

Identifiers

Local EPrints ID: 426657
URI: http://eprints.soton.ac.uk/id/eprint/426657
ISSN: 2469-9926
PURE UUID: 8d51de9f-da24-4f90-a520-e01b1629527a
ORCID for Andrea Vinante: ORCID iD orcid.org/0000-0002-9385-2127

Catalogue record

Date deposited: 07 Dec 2018 18:17
Last modified: 15 Mar 2024 23:07

Export record

Altmetrics

Contributors

Author: Ruchira Mishra
Author: Andrea Vinante ORCID iD
Author: Tejinder Singh

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×