LUNA: Status and prospects
The essential ingredients of nuclear astrophysics are the thermonuclear reactions which
shape the life and death of stars and which are responsible for the synthesis of the chemical …
shape the life and death of stars and which are responsible for the synthesis of the chemical …
Geo-neutrinos and earth's interior
The deepest hole that has ever been dug is about 12km deep. Geochemists analyze
samples from the Earth's crust and from the top of the mantle. Seismology can reconstruct …
samples from the Earth's crust and from the top of the mantle. Seismology can reconstruct …
The experimental nuclear reaction data (EXFOR): Extended computer database and Web retrieval system
Abstract The EXchange FORmat (EXFOR) experimental nuclear reaction database and the
associated Web interface provide access to the wealth of low-and intermediate-energy …
associated Web interface provide access to the wealth of low-and intermediate-energy …
NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number A< 16
Y Xu, K Takahashi, S Goriely, M Arnould, M Ohta… - Nuclear Physics A, 2013 - Elsevier
An update of the NACRE compilation [3] is presented. This new compilation, referred to as
NACRE II, reports thermonuclear reaction rates for 34 charged-particle induced, two-body …
NACRE II, reports thermonuclear reaction rates for 34 charged-particle induced, two-body …
Precision measurement of neutrino oscillation parameters with KamLAND
The KamLAND experiment has determined a precise value for the neutrino oscillation
parameter Δ m 21 2 and stringent constraints on θ 12. The exposure to nuclear reactor …
parameter Δ m 21 2 and stringent constraints on θ 12. The exposure to nuclear reactor …
Constraints on from a three-flavor oscillation analysis of reactor antineutrinos at KamLAND
A Gando, Y Gando, K Ichimura, H Ikeda, K Inoue… - Physical Review D …, 2011 - APS
We present new constraints on the neutrino oscillation parameters Δ m 21 2, θ 12, and θ 13
from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes …
from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes …
Comprehensive geoneutrino analysis with Borexino
M Agostini, K Altenmüller, S Appel, V Atroshchenko… - Physical Review D, 2020 - APS
This paper presents a comprehensive geoneutrino measurement using the Borexino
detector, located at Laboratori Nazionali del Gran Sasso (LNGS) in Italy. The analysis is the …
detector, located at Laboratori Nazionali del Gran Sasso (LNGS) in Italy. The analysis is the …
Direct Measurement of the Cross Section into the -Process Gamow Peak
One of the main neutron sources for the astrophysical s process is the reaction C 13 (α, n) O
16, taking place in thermally pulsing asymptotic giant branch stars at temperatures around …
16, taking place in thermally pulsing asymptotic giant branch stars at temperatures around …
Deep Underground Laboratory Measurement of in the Gamow Windows of the and Processes
B Gao, TY Jiao, YT Li, H Chen, WP Lin, Z An, LH Ru… - Physical Review Letters, 2022 - APS
The C 13 (α, n) O 16 reaction is the main neutron source for the slow-neutron-capture
process in asymptotic giant branch stars and for the intermediate process. Direct …
process in asymptotic giant branch stars and for the intermediate process. Direct …
CIELO collaboration summary results: international evaluations of neutron reactions on uranium, plutonium, iron, oxygen and hydrogen
The CIELO collaboration has studied neutron cross sections on nuclides that significantly
impact criticality in nuclear technologies-235,238 U, 239 Pu, 56 Fe, 16 O and 1 H-with the …
impact criticality in nuclear technologies-235,238 U, 239 Pu, 56 Fe, 16 O and 1 H-with the …