scholarly journals Measurement of High Energy Neutrino–Nucleon Cross Section and Astrophysical Neutrino Flux Anisotropy Study of Cascade Channel with IceCube

2017 ◽  
Author(s):  
Yiqian Xu ◽  
Keyword(s):  
Cross Section ◽  
Neutrino Flux ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino ◽  
Astrophysical Neutrino

scholarly journals Disentangling neutrino-nucleon cross section and high energy neutrino flux with akm3neutrino telescope

2008 ◽  
Vol 77 (4) ◽  
Author(s):  
E. Borriello ◽  
A. Cuoco ◽  
G. Mangano ◽  
G. Miele ◽  
S. Pastor ◽  
...  
Keyword(s):  
Cross Section ◽  
Neutrino Flux ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino

scholarly journals Progress in neutrino astronomy

2021 ◽  
Author(s):  
Carsten Rott
Keyword(s):  
Solar System ◽  
Neutrino Flux ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino ◽  
Neutrino Astronomy ◽  
Astrophysical Neutrino

AbstractThe dream of observing our universe through neutrinos is rapidly becoming a reality. More than three decades after the first observation of neutrinos from beyond our solar system associated with Supernova SN1987A, neutrino astronomy is in the midst of a revolution. Extraterrestrial neutrinos are now routinely detected, following the discovery of a high-energy diffuse astrophysical neutrino flux in 2013. The detection of a high-energy neutrino in coincidence with a flaring blazar in 2017 has brought the field rapidly into the multi-messenger science era. The latest developments in the field of neutrino astronomy are reviewed and prospects with current and future detectors discussed. Particular emphasis is put on domestic programs in neutrino astronomy and the possibility to construct a large neutrino observatory in Korea.

scholarly journals Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert

Science ◽  
2018 ◽  
Vol 361 (6398) ◽  
pp. 147-151 ◽  
Author(s):  
◽  
Mark Aartsen ◽  
Markus Ackermann ◽  
Jenni Adams ◽  
Juan Antonio Aguilar ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Neutrino Flux ◽  
High Energy ◽  
Time Variable ◽  
Neutrino Emission ◽  
High Energy Neutrino ◽  
Excess Emission ◽  
Energy Neutrino ◽  
Variable Flux ◽  
Astrophysical Neutrino

A high-energy neutrino event detected by IceCube on 22 September 2017 was coincident in direction and time with a gamma-ray flare from the blazar TXS 0506+056. Prompted by this association, we investigated 9.5 years of IceCube neutrino observations to search for excess emission at the position of the blazar. We found an excess of high-energy neutrino events, with respect to atmospheric backgrounds, at that position between September 2014 and March 2015. Allowing for time-variable flux, this constitutes 3.5σ evidence for neutrino emission from the direction of TXS 0506+056, independent of and prior to the 2017 flaring episode. This suggests that blazars are identifiable sources of the high-energy astrophysical neutrino flux.

scholarly journals Quantifying uncertainties in the high-energy neutrino cross-section

Pramana ◽  
2012 ◽  
Vol 79 (5) ◽  
pp. 1301-1308 ◽  
Author(s):  
A COOPER-SARKAR ◽  
P MERTSCH ◽  
S SARKAR
Keyword(s):  
Cross Section ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino ◽  
Neutrino Cross Section

scholarly journals Detection of a flaring blazar coincident with an IceCube high-energy neutrino

2019 ◽  
Vol 207 ◽  
pp. 02001
Author(s):  
Anna Franckowiak
Keyword(s):  
Gamma Ray ◽  
Spectral Energy Distribution ◽  
Neutrino Flux ◽  
High Energy ◽  
Spectral Energy ◽  
Large Area ◽  
High Energy Neutrino ◽  
Energy Neutrino ◽  
Radio Wavelength ◽  
First Time

In September 22, 2017, IceCube released a public alert announcing the detection of a 290 TeV neutrino track event with an angular uncertainty of one square degree (90% containment). A multi-messenger follow-up campaign was initiated resulting in the detection of a GeV gamma-ray flare by the Fermi Large Area Telescope positionally consistent with the location of the known Bl Lac object, TXS 0506+056 , located only 0.1 degrees from the best-fit neutrino position. The probability of finding a GeV gamma-ray flare in coincidence with a high-energy neutrino event assuming a correlation of the neutrino flux with the gamma-ray energy flux in the energy band between 1 and 100 GeV was calculated to be 3σ (after trials correction). Following the detection of the flaring blazar the imaging air Cherenkov telescope MAGIC detected the source for the first time in the > 100 GeV gamma-ray band. The activity of the source was confirmed in X-ray, optical and radio wavelength. Several groups have developed lepto-hadronic models which succeed to explain the multi-messenger spectral energy distribution.

High energy neutrino flux from ordinary cosmic strings

1990 ◽  
Vol 331 (1) ◽  
pp. 153-172 ◽  
Author(s):  
Jane H. MacGibbon ◽  
Robert H. Brandenberger
Keyword(s):  
Cosmic Strings ◽  
Neutrino Flux ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino

scholarly journals First constraints on the ultra-high energy neutrino flux from a prototype station of the Askaryan Radio Array

2015 ◽  
Vol 70 ◽  
pp. 62-80 ◽  
Author(s):  
P. Allison ◽  
J. Auffenberg ◽  
R. Bard ◽  
J.J. Beatty ◽  
D.Z. Besson ◽  
...  
Keyword(s):  
Neutrino Flux ◽  
High Energy ◽  
Ultra High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino
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