001     594769
005     20240428052651.0
024 7 _ |a Altavista:2023zhw
|2 INSPIRETeX
024 7 _ |a inspire:2703118
|2 inspire
024 7 _ |a arXiv:2309.14993
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2023-05946
|2 datacite_doi
037 _ _ |a PUBDB-2023-05946
041 _ _ |a English
088 _ _ |a DESY-23-143
|2 DESY
088 _ _ |a arXiv:2309.14993
|2 arXiv
100 1 _ |a Altavista, Chiara
|0 P:(DE-H253)PIP1106783
|b 0
|u desy
245 _ _ |a Induced gravitational waves and baryon asymmetry fluctuations from primordial black hole formation
260 _ _ |c 2023
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1698240676_2148347
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
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336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a 38 pages, 11 figures
520 _ _ |a We consider black hole formation due to the gravitational collapse produced by large density fluctuations during an epoch of reheating with a stiff equation of state and calculate the induced gravitational wave spectrum. By considering the existing bounds on the total energy density of gravitational waves today, we find constraints on the parameter space of this scenario. We also calculate the lepton asymmetry generated by metric perturbations via the chiral gravitational anomaly present in the Standard Model and find that, once the electroweak sphaleron processes have taken place, the large spectrum of scalar perturbations responsible for black hole formation induces a peak in the baryon asymmetry fluctuations on small scales.
536 _ _ |a 611 - Fundamental Particles and Forces (POF4-611)
|0 G:(DE-HGF)POF4-611
|c POF4-611
|f POF IV
|x 0
536 _ _ |a DFG project 390833306 - EXC 2121: Quantum Universe (390833306)
|0 G:(GEPRIS)390833306
|c 390833306
|x 1
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a black hole, formation
|2 INSPIRE
650 _ 7 |a baryon, asymmetry
|2 INSPIRE
650 _ 7 |a gravitational radiation, induced
|2 INSPIRE
650 _ 7 |a metric, perturbation
|2 INSPIRE
650 _ 7 |a gravitation, chiral
|2 INSPIRE
650 _ 7 |a electroweak interaction, sphaleron
|2 INSPIRE
650 _ 7 |a density, fluctuation
|2 INSPIRE
650 _ 7 |a perturbation, scalar
|2 INSPIRE
650 _ 7 |a spectrum, scalar
|2 INSPIRE
650 _ 7 |a anomaly, gravitation
|2 INSPIRE
650 _ 7 |a space-time, perturbation
|2 INSPIRE
650 _ 7 |a energy, density
|2 INSPIRE
650 _ 7 |a lepton, asymmetry
|2 INSPIRE
650 _ 7 |a gravitation, collapse
|2 INSPIRE
650 _ 7 |a gravitational radiation, spectrum
|2 INSPIRE
650 _ 7 |a black hole, primordial
|2 INSPIRE
650 _ 7 |a reheating
|2 INSPIRE
650 _ 7 |a equation of state
|2 INSPIRE
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Rey Idler, Julian Leonardo
|0 P:(DE-H253)PIP1099356
|b 1
|e Corresponding author
|u desy
856 4 _ |u https://bib-pubdb1.desy.de/record/594769/files/HTML-Approval_of_scientific_publication.html
856 4 _ |u https://bib-pubdb1.desy.de/record/594769/files/PDF-Approval_of_scientific_publication.pdf
856 4 _ |y OpenAccess
|u https://bib-pubdb1.desy.de/record/594769/files/2309.14993v1.pdf
856 4 _ |y OpenAccess
|x pdfa
|u https://bib-pubdb1.desy.de/record/594769/files/2309.14993v1.pdf?subformat=pdfa
909 C O |o oai:bib-pubdb1.desy.de:594769
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910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 0
|6 P:(DE-H253)PIP1106783
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 1
|6 P:(DE-H253)PIP1099356
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-611
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Fundamental Particles and Forces
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914 1 _ |y 2023
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
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915 _ _ |a Published
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920 1 _ |0 I:(DE-H253)T-20120731
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|l Theorie-Gruppe
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)T-20120731
980 1 _ |a FullTexts


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