dc.contributor |
Háskóli Íslands |
dc.contributor |
University of Iceland |
dc.contributor.author |
Huang, Guo-yuan |
dc.contributor.author |
Ohlsson, Tommy |
dc.contributor.author |
Zhou, Shun |
dc.date.accessioned |
2019-01-14T11:31:05Z |
dc.date.available |
2019-01-14T11:31:05Z |
dc.date.issued |
2018-04-05 |
dc.identifier.citation |
Huang, G.-y., Ohlsson, T., & Zhou, S. (2018). Observational constraints on secret neutrino interactions from big bang nucleosynthesis. Physical Review D, 97(7), 075009. doi:10.1103/PhysRevD.97.075009 |
dc.identifier.issn |
2470-0010 |
dc.identifier.issn |
2470-0029 (eISSN) |
dc.identifier.uri |
https://hdl.handle.net/20.500.11815/972 |
dc.description |
Publisher's version (útgefin grein) |
dc.description.abstract |
We investigate possible interactions between neutrinos and massive scalar bosons via
g
ϕ
¯
ν
ν
ϕ
(or massive vector bosons via
g
V
¯
ν
γ
μ
ν
V
μ
) and explore the allowed parameter space of the coupling constant
g
ϕ
(or
g
V
) and the scalar (or vector) boson mass
m
ϕ
(or
m
V
) by requiring that these secret neutrino interactions (SNIs) should not spoil the success of big bang nucleosynthesis (BBN). Incorporating the SNIs into the evolution of the early Universe in the BBN era, we numerically solve the Boltzmann equations and compare the predictions for the abundances of light elements with observations. It turns out that the constraint on
g
ϕ
and
m
ϕ
in the scalar-boson case is rather weak, due to a small number of degrees of freedom (d.o.f.). However, in the vector-boson case, the most stringent bound on the coupling
g
V
≲
6
×
10
−
10
at 95% confidence level is obtained for
m
V
≃
1
MeV
, while the bound becomes much weaker
g
V
≲
8
×
10
−
6
for smaller masses
m
V
≲
10
−
4
MeV
. Moreover, we discuss in some detail how the SNIs affect the cosmological evolution and the abundances of the lightest elements. |
dc.description.sponsorship |
This work
was in part supported by the National Natural Science
Foundation of China under Grant No. 11775232, by the
National Recruitment Program for Young Professionals and
the CAS Center for Excellence in Particle Physics
(CCEPP). T. O. acknowledges support by the Swedish
Research Council (Vetenskapsrådet) through Contract
No. 2017-03934 and the KTH Royal Institute of
Technology for a sabbatical period at the University of
Iceland. |
dc.format.extent |
075009 |
dc.language.iso |
en |
dc.publisher |
American Physical Society (APS) |
dc.relation.ispartofseries |
Physical Review D;97(7) |
dc.rights |
info:eu-repo/semantics/openAccess |
dc.subject |
Big bang nucleosynthesis |
dc.subject |
Neutrino interactions |
dc.subject |
Neutrinos |
dc.subject |
Miklihvellur |
dc.subject |
Heimsfræði |
dc.subject |
Atóm |
dc.subject |
Kjarneðlisfræði |
dc.title |
Observational constraints on secret neutrino interactions from big bang nucleosynthesis |
dc.type |
info:eu-repo/semantics/article |
dcterms.license |
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. |
dc.description.version |
Peer Reviewed |
dc.identifier.journal |
Physical Review D |
dc.identifier.doi |
10.1103/PhysRevD.97.075009 |
dc.contributor.department |
Raunvísindastofnun (HÍ) |
dc.contributor.department |
Science Institute (UI) |
dc.contributor.school |
Verkfræði- og náttúruvísindasvið (HÍ) |
dc.contributor.school |
School of Engineering and Natural Sciences (UI) |