Unbroken B–L symmetry

The difference between baryon number B and lepton number L is the only anomaly-free global symmetry of the Standard Model, easily promoted to a local symmetry by introducing three right-handed neutrinos, which automatically make neutrinos massive. The non-observation of any (B–L)-violating processes...

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Main Author: Julian Heeck
Format: Article
Language:English
Published: Elsevier 2014-12-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269314008004
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spelling doaj-74c690634943464c85fbd3a3621fd00e2020-11-24T22:12:53ZengElsevierPhysics Letters B0370-26932014-12-01739256262Unbroken B–L symmetryJulian Heeck0Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany; Institut für Theoretische Physik, Universität Heidelberg, Philosophenweg 16, 69120 Heidelberg, Germany; Correspondence to: Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.The difference between baryon number B and lepton number L is the only anomaly-free global symmetry of the Standard Model, easily promoted to a local symmetry by introducing three right-handed neutrinos, which automatically make neutrinos massive. The non-observation of any (B–L)-violating processes leads us to scrutinize the case of unbroken gauged B–L; besides Dirac neutrinos, the model contains only three parameters, the gauge coupling strength g′, the Stückelberg mass MZ′, and the kinetic mixing angle χ. The new force could manifest itself at any scale, and we collect and derive bounds on g′ over the entire testable range MZ′=0–1013 eV, also of interest for the more popular case of spontaneously broken B–L or other new light forces. We show in particular that successful Big Bang nucleosynthesis provides strong bounds for masses 10 eV<MZ′<10 GeV due to resonant enhancement of the rate f¯f↔ν¯RνR. The strongest limits typically arise from astrophysics and colliders, probing scales MZ′/g′ from TeV up to 1010 GeV.http://www.sciencedirect.com/science/article/pii/S0370269314008004
collection DOAJ
language English
format Article
sources DOAJ
author Julian Heeck
spellingShingle Julian Heeck
Unbroken B–L symmetry
Physics Letters B
author_facet Julian Heeck
author_sort Julian Heeck
title Unbroken B–L symmetry
title_short Unbroken B–L symmetry
title_full Unbroken B–L symmetry
title_fullStr Unbroken B–L symmetry
title_full_unstemmed Unbroken B–L symmetry
title_sort unbroken b–l symmetry
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2014-12-01
description The difference between baryon number B and lepton number L is the only anomaly-free global symmetry of the Standard Model, easily promoted to a local symmetry by introducing three right-handed neutrinos, which automatically make neutrinos massive. The non-observation of any (B–L)-violating processes leads us to scrutinize the case of unbroken gauged B–L; besides Dirac neutrinos, the model contains only three parameters, the gauge coupling strength g′, the Stückelberg mass MZ′, and the kinetic mixing angle χ. The new force could manifest itself at any scale, and we collect and derive bounds on g′ over the entire testable range MZ′=0–1013 eV, also of interest for the more popular case of spontaneously broken B–L or other new light forces. We show in particular that successful Big Bang nucleosynthesis provides strong bounds for masses 10 eV<MZ′<10 GeV due to resonant enhancement of the rate f¯f↔ν¯RνR. The strongest limits typically arise from astrophysics and colliders, probing scales MZ′/g′ from TeV up to 1010 GeV.
url http://www.sciencedirect.com/science/article/pii/S0370269314008004
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