Zobrazeno 1 - 10
of 88
pro vyhledávání: '"van Eijndhoven Nick"'
Autor:
De Kockere, Simon, Broeck, Dieder Van den, Latif, Uzair Abdul, de Vries, Krijn D., van Eijndhoven, Nick, Huege, Tim, Buitink, Stijn
Publikováno v:
Phys. Rev. D 110, 023010 (2024)
A new generation of neutrino observatories will search for PeV-EeV neutrinos interacting in the ice by detecting radio pulses. Extended air showers propagating into the ice will form an important background and could be a valuable calibration signal.
Externí odkaz:
http://arxiv.org/abs/2403.15358
Autor:
Merckx, Yarno, Correa, Pablo, de Vries, Krijn D., Kotera, Kumiko, Privon, George C., van Eijndhoven, Nick
Publikováno v:
Phys. Rev. D 108 (2023) 023015
We present a phenomenological framework for starburst-driven neutrino production via proton-proton collisions and apply it to (ultra)luminous infrared galaxies (U/LIRGs) in the Great Observatories All-Sky LIRG Survey (GOALS). The framework relates th
Externí odkaz:
http://arxiv.org/abs/2304.01020
Autor:
de Vries Krijn D., Buitink Stijn, van Eijndhoven Nick, Meures Thomas, O’Murchadha Aongus, Scholten Olaf
Publikováno v:
EPJ Web of Conferences, Vol 135, p 05001 (2017)
We discuss the radio emission from a cosmic-ray air shower propagating in air before it hits an air-ice boundary after which it completes its propagation inside the ice. The in-air emission, the in-ice emission, as well as the transition radiation fr
Externí odkaz:
https://doaj.org/article/4ab9729a81794aff8b4086fa3413a19d
Publikováno v:
EPJ Web of Conferences, Vol 135, p 05006 (2017)
We discuss the radar detection method as a probe for high-energy neutrino induced particle cascades in ice. In a previous work we showed that the radar detection techniqe is a promising method to probe the high-energy cosmic neutrino flux above PeV e
Externí odkaz:
https://doaj.org/article/fe68327465104f83bbcd9eae282c7c72
Publikováno v:
Phys. Rev. D 106, 043023 (2022)
We present detailed microscopic simulations of high-energy cosmic-ray air showers penetrating high-altitude ice layers that can be found at the polar regions. We use a combination of the CORSIKA Monte Carlo code and the Geant4 simulation toolkit, and
Externí odkaz:
http://arxiv.org/abs/2202.09211
Currently new radio detection techniques are being explored to detect astrophysical neutrinos beyond the PeV scale interacting in polar ice. Due to the long attenuation length of radio waves in a medium, it can be expected that such instruments will
Externí odkaz:
http://arxiv.org/abs/2202.08754
With infrared luminosities $L_{\mathrm{IR}} \geq 10^{12} L_{\odot}$, Ultra-Luminous Infrared Galaxies (ULIRGs) are the most luminous objects in the infrared sky. They are predominantly powered by starburst regions with star-formation rates $\gtrsim 1
Externí odkaz:
http://arxiv.org/abs/2107.08422
Publikováno v:
Phys. Rev. D 102, 103014 (2020)
We present an analysis of more than 11 years of Fermi-GBM data in which 217 Gamma-Ray Bursts (GRBs) are found for which their main burst is preceded by a precursor flash. We find that short GRBs ($<$2 s) are ~10 times less likely to produce a precurs
Externí odkaz:
http://arxiv.org/abs/2004.03246
Autor:
Coppin, Paul, van Eijndhoven, Nick
While gamma-ray bursts (GRBs) were once believed to be a dominant source of astrophysical neutrinos, the lack of any significant correlation between high-energy photons and neutrinos has resulted in stringent limits on their neutrino fluxes. Previous
Externí odkaz:
http://arxiv.org/abs/1908.06653
Autor:
Glaser, Christian, García-Fernández, Daniel, Nelles, Anna, Alvarez-Muñiz, Jaime, Barwick, Steven W., Besson, Dave Z., Clark, Brian A., Connolly, Amy, Deaconu, Cosmin, de Vries, Krijn, Hanson, Jordan C., Hokanson-Fasig, Ben, Lahmann, R., Latif, Uzair, Kleinfelder, Stuart A., Persichilli, Christopher, Pan, Yue, Pfender, Carl, Plaisier, Ilse, Seckel, Dave, Torres, Jorge, Toscano, Simona, van Eijndhoven, Nick, Vieregg, Abigail, Welling, Christoph, Winchen, Tobias, Wissel, Stephanie A.
Publikováno v:
Eur. Phys. J. C 80, 77 (2020)
NuRadioMC is a Monte Carlo framework designed to simulate ultra-high energy neutrino detectors that rely on the radio detection method. This method exploits the radio emission generated in the electromagnetic component of a particle shower following
Externí odkaz:
http://arxiv.org/abs/1906.01670