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NSR database version of April 26, 2024.

Search: Author = R.Saldanha

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2021AV04      Phys.Rev. D 104, 112007 (2021)

A.Avasthi, T.W.Bowyer, C.Bray, T.Brunner, N.Catarineu, E.Church, R.Guenette, S.J.Haselschwardt, J.C.Hayes, M.Heffner, S.A.Hertel, P.H.Humble, A.Jamil, S.H.Kim, R.F.Lang, K.G.Leach, B.G.Lenardo, W.H.Lippincott, A.Marino, D.N.McKinsey, E.H.Miller, D.C.Moore, B.Mong, B.Monreal, M.E.Monzani, I.Olcina, J.L.Orrell, S.Pang, A.Pocar, P.C.Rowson, R.Saldanha, S.Sangiorgio, C.Stanford, A.Visser

Kiloton-scale xenon detectors for neutrinoless double beta decay and other new physics searches

RADIOACTIVITY ^134,136Xe(2β^-); analyzed available data; deduced neutrinoless mode T_1/2 limits.

doi: 10.1103/PhysRevD.104.112007
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2019SA41      Phys.Rev. C 100, 024608 (2019)

R.Saldanha, H.O.Back, R.H.M.Tsang, T.Alexander, S.R.Elliott, S.Ferrara, E.Mace, C.Overman, M.Zalavadia

Cosmogenic production of ³⁹Ar and ³⁷Ar in argon

NUCLEAR REACTIONS ⁴⁰Ar(n, 2n)³⁹Ar, ⁴⁰Ar(n, d)³⁹Cl, ⁴⁰Ar(n, 4n)³⁷Ar, E=10-1000 MeV; measured Eβ using sensitive ultralow background proportional counters; deduced cross sections, production rates for ³⁷Ar and ³⁹Ar; estimated total cosmogenic production rates for ³⁹Ar from cosmic ray neutrons, protons and muons at sea level. Comparison with previous experimental measurements, and different cross-section models: TALYS, TENDL-1015, MENDEL-2P and INCL++ (ABLA07). Natural Ar samples were irradiated with fast neutrons at the LANSCE WNR ICE-HOUSE II facility. Relevance to argon-based dark matter experiments.

NUCLEAR REACTIONS ⁴⁰Ar(γ, n), (p, pn), (n, 2n)³⁹Ar, E=10-1000 MeV; ³⁸Ar(nγ)³⁹Ar, E=0.001 eV-10 MeV; ⁴⁰Ar(γ, p), (n, d), (γ, 3n), (p, 2p), (μ, n)³⁹Cl, E=10-1000 MeV; ⁴⁰Ar(γ, 3n), (p, 3np)³⁷Ar; ³⁶Ar(n, γ)³⁷Ar, E=0.001 eV-10 MeV; ³⁸Ar(n, 2n), (γ, n), (p, np)³⁷Ar; ⁴⁰Ar(n, 4n), (γ, 3n), (p, 3np)³⁷Ar; compiled experimental data for reactions, and compared to different cross section models such as TALYS and with evaluated data in ENDF/B-VIII.I to estimated total production rates of cosmogenic ³⁷Ar and ³⁹Ar.

doi: 10.1103/PhysRevC.100.024608
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