activity
20022026
most citedFirst Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance

2.7k citations · 12.2k across the 169 of their papers we have counts for

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Showing 2015Show all

15 papers · 1 filter

physics.ins-det2015

Status Update of the MAJORANA DEMONSTRATOR Neutrinoless Double Beta Decay Experiment

Julieta Gruszko, Nicolas Abgrall, Isaac Arnquist +67

Neutrinoless double beta decay searches play a major role in determining neutrino properties, in particular the Majorana or Dirac nature of the neutrino and the absolute scale of t…

physics.ins-det2015★ 26 cited

The COHERENT Experiment at the Spallation Neutron Source

COHERENT Collaboration, D. Akimov, P. An +64

The COHERENT collaboration's primary objective is to measure coherent elastic neutrino-nucleus scattering (CEvNS) using the unique, high-quality source of tens-of-MeV neutrinos pro…

physics.ins-det2015★ 1 cited

Status of the MAJORANA DEMONSTRATOR

C. Cuesta, N. Abgrall, I. J. Arnquist +67

The MAJORANA Collaboration is constructing the MAJORANA DEMONSTRATOR, an ultra-low background, modular, HPGe detector array with a mass of 44-kg (29 kg 76Ge and 15 kg natGe) to sea…

physics.ins-det2015★ 1 cited

Low Background Signal Readout Electronics for the MAJORANA DEMONSTRATOR

I. Guinn, N. Abgrall, I. J. Arnquist +65

The MAJORANA Collaboration will seek neutrinoless double beta decay (0nbb) in 76Ge using isotopically enriched p-type point contact (PPC) high purity Germanium (HPGe) detectors. A…

physics.ins-det2015

Analysis techniques for background rejection at the MAJORANA DEMONSTRATOR

C. Cuesta, N. Abgrall, I. J. Arnquist +65

The MAJORANA Collaboration is constructing the MAJORANA DEMONSTRATOR, an ultra-low background, 40-kg modular HPGe detector array to search for neutrinoless double beta decay in 76G…

astro-ph.HE2015★ 66 cited

KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars

K. Asakura, A. Gando, Y. Gando +44

In the late stages of nuclear burning for massive stars ($M>8~M_{\sun}$), the production of neutrino-antineutrino pairs through various processes becomes the dominant stellar cooli…