Astrophysical neutrinos at the low and high energy frontiers

abstract: For this project, the diffuse supernova neutrino background (DSNB) has been calculated based on the recent direct supernova rate measurements and neutrino spectrum from SN1987A. The estimated diffuse electron antineutrino flux is ∼ 0.10 – 0.59 /cm2/s at 99% confidence lev...

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Other Authors: Yang, Lili (Author)
Format: Doctoral Thesis
Language:English
Published: 2013
Subjects:
Online Access:http://hdl.handle.net/2286/R.I.20985
id ndltd-asu.edu-item-20985
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spelling ndltd-asu.edu-item-209852018-06-22T03:04:42Z Astrophysical neutrinos at the low and high energy frontiers abstract: For this project, the diffuse supernova neutrino background (DSNB) has been calculated based on the recent direct supernova rate measurements and neutrino spectrum from SN1987A. The estimated diffuse electron antineutrino flux is ∼ 0.10 – 0.59 /cm2/s at 99% confidence level, which is 5 times lower than the Super-Kamiokande 2012 upper limit of 3.0 /cm2/s, above energy threshold of 17.3 MeV. With a Megaton scale water detector, 40 events could be detected above the threshold per year. In addition, the detectability of neutrino bursts from direct black hole forming collapses (failed supernovae) at Megaton detectors is calculated. These neutrino bursts are energetic and with short time duration, ∼ 1s. They could be identified by the time coincidence of N ≥2 or N ≥3 events within 1s time window from nearby (4 – 5 Mpc) failed supernovae. The detection rate of these neutrino bursts could get up to one per decade. This is a realistic way to detect a failed supernova and gives a promising method for studying the physics of direct black hole formation mechanism. Finally, the absorption of ultra high energy (UHE) neutrinos by the cosmic neutrino background, with full inclusion of the effect of the thermal distribution of the background on the resonant annihilation channel, is discussed. Results are applied to serval models of UHE neutrino sources. Suppression effects are strong for sources that extend beyond z ∼ 10. This provides a fascinating probe of the physics of the relic neutrino background in the unexplored redshift interval z ∼ 10 – 100. Ultimately this research will examine the detectability of DSNB, neutrino bursts from failed supernovae and absorption effects in the neutrino spectrum. Dissertation/Thesis Yang, Lili (Author) Lunardini, Cecilia (Advisor) Alarcon, Ricardo (Committee member) Shovkovy, Igor (Committee member) Timmes, Francis (Committee member) Vachaspati, Tanmay (Committee member) Arizona State University (Publisher) Physics Astrophysics Diffuse flux Failed supernova Neutrino Supernova Ultra-high energy eng 129 pages Ph.D. Physics 2013 Doctoral Dissertation http://hdl.handle.net/2286/R.I.20985 http://rightsstatements.org/vocab/InC/1.0/ All Rights Reserved 2013
collection NDLTD
language English
format Doctoral Thesis
sources NDLTD
topic Physics
Astrophysics
Diffuse flux
Failed supernova
Neutrino
Supernova
Ultra-high energy
spellingShingle Physics
Astrophysics
Diffuse flux
Failed supernova
Neutrino
Supernova
Ultra-high energy
Astrophysical neutrinos at the low and high energy frontiers
description abstract: For this project, the diffuse supernova neutrino background (DSNB) has been calculated based on the recent direct supernova rate measurements and neutrino spectrum from SN1987A. The estimated diffuse electron antineutrino flux is ∼ 0.10 – 0.59 /cm2/s at 99% confidence level, which is 5 times lower than the Super-Kamiokande 2012 upper limit of 3.0 /cm2/s, above energy threshold of 17.3 MeV. With a Megaton scale water detector, 40 events could be detected above the threshold per year. In addition, the detectability of neutrino bursts from direct black hole forming collapses (failed supernovae) at Megaton detectors is calculated. These neutrino bursts are energetic and with short time duration, ∼ 1s. They could be identified by the time coincidence of N ≥2 or N ≥3 events within 1s time window from nearby (4 – 5 Mpc) failed supernovae. The detection rate of these neutrino bursts could get up to one per decade. This is a realistic way to detect a failed supernova and gives a promising method for studying the physics of direct black hole formation mechanism. Finally, the absorption of ultra high energy (UHE) neutrinos by the cosmic neutrino background, with full inclusion of the effect of the thermal distribution of the background on the resonant annihilation channel, is discussed. Results are applied to serval models of UHE neutrino sources. Suppression effects are strong for sources that extend beyond z ∼ 10. This provides a fascinating probe of the physics of the relic neutrino background in the unexplored redshift interval z ∼ 10 – 100. Ultimately this research will examine the detectability of DSNB, neutrino bursts from failed supernovae and absorption effects in the neutrino spectrum. === Dissertation/Thesis === Ph.D. Physics 2013
author2 Yang, Lili (Author)
author_facet Yang, Lili (Author)
title Astrophysical neutrinos at the low and high energy frontiers
title_short Astrophysical neutrinos at the low and high energy frontiers
title_full Astrophysical neutrinos at the low and high energy frontiers
title_fullStr Astrophysical neutrinos at the low and high energy frontiers
title_full_unstemmed Astrophysical neutrinos at the low and high energy frontiers
title_sort astrophysical neutrinos at the low and high energy frontiers
publishDate 2013
url http://hdl.handle.net/2286/R.I.20985
_version_ 1718700293299896320