Neutrinos from gamma ray bursts in the IceCube and ARA era

Dafne Guetta

doi:10.1016/j.jheap.2015.03.004

Neutrinos from gamma ray bursts in the IceCube and ARA era

Research output: Contribution to journal › Review article › peer-review

Abstract

In this review I discuss the ultra-high energy neutrinos (UHEN) originated from cosmic-ray propagation (GZK neutrinos) and from Gamma Ray Bursts (GRBs), and discuss their detectability in kilometers scale detectors like ARA and IceCube. While GZK neutrinos are expected from cosmic ray interactions on the CMB, the GRB neutrinos depend on the physics inside the sources. GRBs are predicted to emit UHEN in the prompt and in the later 'after-glow' phase. I discuss the constraints on the hadronic component of GRBs derived from the search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs) and more in general I present the results of the search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2013.

Original language	English
Pages (from-to)	90-94
Number of pages	5
Journal	Journal of High Energy Astrophysics
Volume	7
DOIs	https://doi.org/10.1016/j.jheap.2015.03.004
State	Published - 1 Sep 2015
Externally published	Yes

Keywords

Gamma-ray bursts
Neutrino astronomy

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1016/j.jheap.2015.03.004

Cite this

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title = "Neutrinos from gamma ray bursts in the IceCube and ARA era",

abstract = "In this review I discuss the ultra-high energy neutrinos (UHEN) originated from cosmic-ray propagation (GZK neutrinos) and from Gamma Ray Bursts (GRBs), and discuss their detectability in kilometers scale detectors like ARA and IceCube. While GZK neutrinos are expected from cosmic ray interactions on the CMB, the GRB neutrinos depend on the physics inside the sources. GRBs are predicted to emit UHEN in the prompt and in the later 'after-glow' phase. I discuss the constraints on the hadronic component of GRBs derived from the search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs) and more in general I present the results of the search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2013.",

keywords = "Gamma-ray bursts, Neutrino astronomy",

author = "Dafne Guetta",

note = "Publisher Copyright: {\textcopyright} 2015 Elsevier B.V.",

year = "2015",

month = sep,

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doi = "10.1016/j.jheap.2015.03.004",

language = "الإنجليزيّة",

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AB - In this review I discuss the ultra-high energy neutrinos (UHEN) originated from cosmic-ray propagation (GZK neutrinos) and from Gamma Ray Bursts (GRBs), and discuss their detectability in kilometers scale detectors like ARA and IceCube. While GZK neutrinos are expected from cosmic ray interactions on the CMB, the GRB neutrinos depend on the physics inside the sources. GRBs are predicted to emit UHEN in the prompt and in the later 'after-glow' phase. I discuss the constraints on the hadronic component of GRBs derived from the search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs) and more in general I present the results of the search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2013.

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KW - Neutrino astronomy

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U2 - 10.1016/j.jheap.2015.03.004

DO - 10.1016/j.jheap.2015.03.004

M3 - مقالة مرجعية

SN - 2214-4048

VL - 7

SP - 90

EP - 94

JO - Journal of High Energy Astrophysics

JF - Journal of High Energy Astrophysics

ER -

Neutrinos from gamma ray bursts in the IceCube and ARA era

Abstract

Keywords

All Science Journal Classification (ASJC) codes

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