Thermal excitation spectrum from entanglement in an expanding quantum string

A surprising result in e+e− collisions is that the particle spectra from the string formed between the expanding quark–antiquark pair have thermal properties even though scatterings appear not to be frequent enough to explain this. We address this problem by considering the finite observable interva...

Full description

Bibliographic Details
Main Authors: Jürgen Berges, Stefan Floerchinger, Raju Venugopalan
Format: Article
Language:English
Published: Elsevier 2018-03-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269318300868
id doaj-2e415693da0749249d915ae884141ac5
record_format Article
spelling doaj-2e415693da0749249d915ae884141ac52020-11-25T01:00:18ZengElsevierPhysics Letters B0370-26931873-24452018-03-01778C44244610.1016/j.physletb.2018.01.068Thermal excitation spectrum from entanglement in an expanding quantum stringJürgen Berges0Stefan Floerchinger1Raju Venugopalan2Institut für Theoretische Physik, Universität Heidelberg, Philosophenweg 16, 69120 Heidelberg, GermanyInstitut für Theoretische Physik, Universität Heidelberg, Philosophenweg 16, 69120 Heidelberg, GermanyPhysics Department, Brookhaven National Laboratory, Bldg. 510A, Upton, NY 11973, USAA surprising result in e+e− collisions is that the particle spectra from the string formed between the expanding quark–antiquark pair have thermal properties even though scatterings appear not to be frequent enough to explain this. We address this problem by considering the finite observable interval of a relativistic quantum string in terms of its reduced density operator by tracing over the complement region. We show how quantum entanglement in the presence of a horizon in spacetime for the causal transfer of information leads locally to a reduced mixed-state density operator. For very early proper time τ, we show that the entanglement entropy becomes extensive and scales with the rapidity. At these early times, the reduced density operator is of thermal form, with an entanglement temperature Tτ=ħ/(2πkBτ), even in the absence of any scatterings.http://www.sciencedirect.com/science/article/pii/S0370269318300868
collection DOAJ
language English
format Article
sources DOAJ
author Jürgen Berges
Stefan Floerchinger
Raju Venugopalan
spellingShingle Jürgen Berges
Stefan Floerchinger
Raju Venugopalan
Thermal excitation spectrum from entanglement in an expanding quantum string
Physics Letters B
author_facet Jürgen Berges
Stefan Floerchinger
Raju Venugopalan
author_sort Jürgen Berges
title Thermal excitation spectrum from entanglement in an expanding quantum string
title_short Thermal excitation spectrum from entanglement in an expanding quantum string
title_full Thermal excitation spectrum from entanglement in an expanding quantum string
title_fullStr Thermal excitation spectrum from entanglement in an expanding quantum string
title_full_unstemmed Thermal excitation spectrum from entanglement in an expanding quantum string
title_sort thermal excitation spectrum from entanglement in an expanding quantum string
publisher Elsevier
series Physics Letters B
issn 0370-2693
1873-2445
publishDate 2018-03-01
description A surprising result in e+e− collisions is that the particle spectra from the string formed between the expanding quark–antiquark pair have thermal properties even though scatterings appear not to be frequent enough to explain this. We address this problem by considering the finite observable interval of a relativistic quantum string in terms of its reduced density operator by tracing over the complement region. We show how quantum entanglement in the presence of a horizon in spacetime for the causal transfer of information leads locally to a reduced mixed-state density operator. For very early proper time τ, we show that the entanglement entropy becomes extensive and scales with the rapidity. At these early times, the reduced density operator is of thermal form, with an entanglement temperature Tτ=ħ/(2πkBτ), even in the absence of any scatterings.
url http://www.sciencedirect.com/science/article/pii/S0370269318300868
work_keys_str_mv AT jurgenberges thermalexcitationspectrumfromentanglementinanexpandingquantumstring
AT stefanfloerchinger thermalexcitationspectrumfromentanglementinanexpandingquantumstring
AT rajuvenugopalan thermalexcitationspectrumfromentanglementinanexpandingquantumstring
_version_ 1725214195315638272