Results 101 to 110 of about 19,659 (274)

Current Direct Neutrino Mass Experiments

Advances in High Energy Physics, Volume 2013, Issue 1, 2013., 2013
In this contribution, we review the status and perspectives of direct neutrino mass experiments, which investigate the kinematics of β‐decays of specific isotopes (3H, 187Re, 163Ho) to derive model‐independent information on the averaged electron (anti)neutrino mass. After discussing the kinematics of β‐decay and the determination of the neutrino mass,
G. Drexlin, V. Hannen, S. Mertens, C. Weinheimer, Arthur B. McDonald   +4 more
wiley   +1 more source

The Pierre Auger Observatory status and latest results

EPJ Web of Conferences, 2017
The Pierre Auger Observatory, in Argentina, is the present flagship experiment studying ultrahigh-energy cosmic rays (UHECRs). Facing the challenge due to low cosmic-ray flux at the highest energies, the Observatory has been taking data for more than a ...
Berat Corinne
doaj   +1 more source

Ultra-high energy neutrinos searches with the Pierre Auger Observatory

SciPost Physics Proceedings, 2019
In the EeV range, neutrinos are expected to be produced by ultra-high energy cosmic rays interactions with the Cosmic Microwave Background during propagation in the Universe.
Marta Trini for the Pierre Auger Collaboration
doaj   +1 more source

Origin of atmospheric aerosols at the Pierre Auger Observatory using backward trajectory of air masses

, 2012
The Pierre Auger Observatory is the largest operating cosmic ray observatory ever built. Calorimetric measurements of extensive air showers induced by cosmic rays are performed with a fluorescence detector.
, Abreu P [Pierre Auger Collaboration], Fick B, GD Rolph, Karim Louedec, Louedec K, MI Micheletti, RR Draxler   +7 more
core   +3 more sources

The rate of cosmic ray showers at large zenith angles: a step towards the detection of ultra-high energy neutrinos by the Pierre Auger Observatory [PDF]

, 2000
It is anticipated that the Pierre Auger Observatory can be used to detect cosmic neutrinos of >10^19 eV that arrive at very large zenith angles.
A.A. Watson, Antoni, Bird, Capelle, E. Zas, Edge, Engel, Fletcher, J.A. Hinton, Kalmykov, Kalmykov, Kalmykov, Lawrence, M. Ave, Mikamo, Nagano, Nagano, Navarra, R.A. Vázquez, Tennent, Zas   +20 more
core   +2 more sources

Thank You to Our 2024 Reviewers

Geophysical Research Letters, Volume 52, Issue 4, 28 February 2025.
Abstract On behalf of the journal, AGU, and the scientific community, the editors of Geophysical Research Letters would like to sincerely thank those who reviewed manuscripts in 2024. The hours reading and commenting on manuscripts not only improve the manuscripts but also increase the scientific rigor of future research in the field.
Kris Karnauskas, Anantha Aiyyer, Suzana Camargo, Fabio Capitanio, Sarah Feakins, Robinson Fulweiler, Neil Ganju, Alessandra Giannini, Yu Gu, Christian Huber, Valeriy Ivanov, Monika Korte, Sujay Kumar, Kevin Lewis, Gudrun Magnusdottir, Mathieu Morlighem, Yuichi Otsuka, Germán A. Prieto, Bo Qiu, Lynn Russell, Kanako Seki, Hui Su, Daoyuan Sun, Hari Viswanathan, Guiling Wang, Kaicun Wang, Angelicque E. White, Quentin Williams, Lei Zhang   +28 more
wiley   +1 more source

The Pierre Auger Observatory highlights [PDF]

Proceedings of XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop — PoS(MULTIF2017), 2018
In the past decade the number of ultra-high energy cosmic rays detected has increased enormously. This is mostly due to the operation of the Pierre Auger Observatory, in Argentina, the largest cosmic ray detector ever built. Through this detector we now know better the most energetic particles in the universe, we can now start to answer some of the ...
openaire   +1 more source

The Auger Raman Lidar: several years of continuous observations

EPJ Web of Conferences, 2019
The Raman lidar at the Central (Raman) Laser Facility of the Pierre Auger Observatory in Argentina, has been operational since September 2013. In this paper, the Auger Raman Lidar performance is discussed in terms of the data quality for the assessment ...
Rizi Vincenzo, Hernandez Carlos Medina, Iarlori Marco, Pietropaolo Ermanno   +3 more
doaj   +1 more source

Signature of Plausible Accreting Supermassive Black Holes in Mrk 261/262 and Mrk 266

Advances in Astronomy, Volume 2013, Issue 1, 2013., 2013
We address the neutrino radiation of plausible accreting supermassive black holes closely linking to the 5 nuclear components of galaxy samples of Mrk 261/262 and Mrk 266. We predict a time delay before neutrino emission of the same scale as the age of the Universe. The ultrahigh energy neutrinos are produced in superdense protomatter medium via simple
Gagik Ter-Kazarian, Lusine Sargsyan, William Reach   +2 more
wiley   +1 more source

Measurements of Horizontal Air Showers with the Auger Engineering Radio Array [PDF]

EPJ Web of Conferences, 2019
The Pierre Auger Observatory is the largest observatory for the detection of cosmic rays. With the Auger Engineering Radio Array (AERA) we measure the emitted radio signal of extensive air showers and reconstruct properties of the primary cosmic rays ...
Gottowik Marvin
doaj   +1 more source