Results 121 to 130 of about 6,622 (234)
Constraints on Dark Photon from Neutrino-Electron Scattering Experiments
A possible manifestation of an additional light gauge boson $A^\prime$, named as Dark Photon, associated with a group $U(1)_{\rm B-L}$ is studied in neutrino electron scattering experiments.
Aliev, T. M. +5 more
core +2 more sources
Luminous signals of inelastic dark matter in large detectors
We study luminous dark matter signals in models with inelastic scattering. Dark matter χ 1 that scatters inelastically off elements in the Earth is kicked into an excited state χ 2 that can subsequently decay into a monoenergetic photon inside a detector.
Joshua Eby +3 more
doaj +1 more source
Solar Neutrino Matter Effects Redux
Following recent low-threshold analysis of the Sudbury Neutrino Observatory and asymmetry measurements of the BOREXINO Collaboration of the solar neutrino flux, we revisit the analysis of the matter effects in the Sun.
A. B. Balantekin +3 more
core +1 more source
Status of the Borexino experiment
2 pages, 1 figure; uses moriond.sty (attached), epsfig and picinpar packages; to appear in proceeding of the Rencontres de Moriond conference, Electroweak and Unified Theories session ...
openaire +3 more sources
Measurement of geo-neutrinos from 1353 days of Borexino [PDF]
G. Bellini +92 more
openalex +1 more source
Mono-lepton signature of a neutrino-philic dark fermion at hadron colliders
Searching for dark matter at high-energy colliders and direct detection experiments can effectively cover nearly the entire mass range from the MeV to the TeV scale.
Kai Ma, Lin-Yun He
doaj +1 more source
Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino [PDF]
S. Appel +78 more
semanticscholar +1 more source
Neutrinos and (Anti)neutrinos from Supernovae and from the Earth in the Borexino detector
The main goal of the Borexino detector, in its final phase of construction in the Gran Sasso underground laboratory, is the direct observation and measurement of the low energy component of neutrinos coming from the Sun. The unique low energy sensitivity
Miramonti, Lino
core
Source insertion & location systems for the Borexino solar neutrino detector [PDF]
Steve Hardy +4 more
openalex +1 more source

