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NSR database version of April 11, 2024.

Search: Author = E.Miller

Found 5 matches.

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2021AK04      Phys.Rev. C 104, 065501 (2021)

D.S.Akerib, A.K.Al Musalhi, S.K.Alsum, C.S.Amarasinghe, A.Ames, T.J.Anderson, N.Angelides, H.M.Araujo, J.E.Armstrong, M.Arthurs, X.Bai, J.Balajthy, S.Balashov, J.Bang, J.W.Bargemann, D.Bauer, A.Baxter, P.Beltrame, E.P.Bernard, A.Bernstein, A.Bhatti, A.Biekert, T.P.Biesiadzinski, H.J.Birch, G.M.Blockinger, E.Bodnia, B.Boxer, C.A.J.Brew, P.Bras, S.Burdin, J.K.Busenitz, M.Buuck, R.Cabrita, M.C.Carmona-Benitez, M.Cascella, C.Chan, N.I.Chott, A.Cole, M.V.Converse, A.Cottle, G.Cox, O.Creaner, J.E.Cutter, C.E.Dahl, L.de Viveiros, J.E.Y.Dobson, E.Druszkiewicz, S.R.Eriksen, A.Fan, S.Fayer, N.M.Fearon, S.Fiorucci, H.Flaecher, E.D.Fraser, T.Fruth, R.J.Gaitskell, J.Genovesi, C.Ghag, E.Gibson, S.Gokhale, M.G.D.van der Grinten, C.B.Gwilliam, C.R.Hall, S.J.Haselschwardt, S.A.Hertel, M.Horn, D.Q.Huang, M.C.I.gnarra, O.Jahangir, R.S.James, W.Ji, J.Johnson, A.C.Kaboth, A.C.Kamaha, K.Kamdin, K.Kazkaz, D.Khaitan, A.Khazov, I.Khurana, D.Kodroff, L.Korley, E.V.Korolkova, H.Kraus, S.Kravitz, L.Kreczko, B.Krikler, V.A.Kudryavtsev, E.A.Leason, J.Lee, D.S.Leonard, K.T.Lesko, C.Levy, J.Liao, J.Lin, A.Lindote, R.Linehan, W.H.Lippincott, X.Liu, M.I.Lopes, E.Lopez Asamar, B.Lopez Paredes, W.Lorenzon, S.Luitz, P.A.Majewski, A.Manalaysay, L.Manenti, R.L.Mannino, N.Marangou, M.E.McCarthy, D.N.McKinsey, J.McLaughlin, E.H.Miller, E.Mizrachi, A.Monte, M.E.Monzani, J.A.Morad, J.D.Morales Mendoza, E.Morrison, B.J.Mount, A.St.J.Murphy, D.Naim, A.Naylor, C.Nedlik, H.N.Nelson, F.Neves, J.A.Nikoleyczik, A.Nilima, I.Olcina, K.C.Oliver-Mallory, S.Pal, K.J.Palladino, J.Palmer, S.Patton, N.Parveen, E.K.Pease, B.Penning, G.Pereira, A.Piepke, Y.Qie, J.Reichenbacher, C.A.Rhyne, A.Richards, Q.Riffard, G.R.C.Rischbieter, R.Rosero, P.Rossiter, D.Santone, A.B.M.R.Sazzad, R.W.Schnee, P.R.Scovell, S.Shaw, T.A.Shutt, J.J.Silk, C.Silva, R.Smith, M.Solmaz, V.N.Solovov, P.Sorensen, J.Soria, I.Stancu, A.Stevens, K.Stifter, B.Suerfu, T.J.Sumner, N.Swanson, M.Szydagis, W.C.Taylor, R.Taylor, D.J.Temples, P.A.Terman, D.R.Tiedt, M.Timalsina, W.H.To, D.R.Tovey, M.Tripathi, D.R.Tronstad, W.Turner, U.Utku, A.Vaitkus, B.Wang, J.J.Wang, W.Wang, J.R.Watson, R.C.Webb, R.G.White, T.J.Whitis, M.Williams, F.L.H.Wolfs, D.Woodward, C.J.Wright, X.Xiang, J.Xu, M.Yeh, P.Zarzhitsky

Projected sensitivity of the LUX-ZEPLIN experiment to the two-neutrino and neutrinoless double β decays of 134Xe

RADIOACTIVITY 134Xe(2β-); measured recoiling nuclei and electrons, decay energy spectra using LUX-ZEPLIN (LZ) detector of liquid xenon (LXe), with scintillation and electro-luminescence light detected using 494 photomultipliers at Sanford Underground Research Facility (SURF) in South Dakota; deduced lower limits of T1/2 values for 2νββ and 0νββ decay modes.

doi: 10.1103/PhysRevC.104.065501
Citations: PlumX Metrics


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 T1/2 limits.

doi: 10.1103/PhysRevD.104.112007
Citations: PlumX Metrics


2021HO14      Phys.Rev. C 104, 024610 (2021)

C.J.Horsfield, M.S.Rubery, J.M.Mack, H.W.Herrmann, Y.Kim, C.S.Young, S.E.Caldwell, S.C.Evans, T.S.Sedillo, A.M.McEvoy, N.M.Hoffman, M.A.Huff, J.R.Langenbrunner, G.M.Hale, D.C.Wilson, W.Stoeffl, J.A.Church, E.M.Grafil, E.K.Miller, V.Y.Glebov

First spectral measurement of deuterium-tritium fusion γ rays in inertial fusion experiments

NUCLEAR REACTIONS 3H(d, γ)5He*, E not given; measured fusion Eγ, Iγ from deuterium-tritium (DT) inertial confinement fusion (ICF) implosions with Omega laser, branching ratio of γ rays from transitions to an intermediate excited state and the ground state using R-matrix analysis.

doi: 10.1103/PhysRevC.104.024610
Citations: PlumX Metrics


2012KI10      Phys.Rev. C 85, 061601 (2012)

Y.Kim, J.M.Mack, H.W.Herrmann, C.S.Young, G.M.Hale, S.Caldwell, N.M.Hoffman, S.C.Evans, T.J.Sedillo, A.McEvoy, J.Langenbrunner, H.H.Hsu, M.A.Huff, S.Batha, C.J.Horsfield, M.S.Rubery, W.J.Garbett, W.Stoeffl, E.Grafil, L.Bernstein, J.A.Church, D.B.Sayre, M.J.Rosenberg, C.Waugh, H.G.Rinderknecht, M.G.Johnson, A.B.Zylstra, J.A.Frenje, D.T.Casey, R.D.Petrasso, E.K.Miller, V.Yu.Glebov, C.Stoeckl, T.C.Sangster

Determination of the deuterium-tritium branching ratio based on inertial confinement fusion implosions

NUCLEAR REACTIONS 3H(d, γ)5He, 3H(d, n)4He, E(cm)=14-24 keV; measured absolute neutron and γ-ray yields in inertial confinement fusion (ICF) conditions; deduced branching ratio of γ-to-neutron in d+t reaction. Measurement of γ-to-proton branching ratio in 3He(d, γ)5Li and 3He(d, p)4He reactions used for cross calibration. Comparison with previous studies.

doi: 10.1103/PhysRevC.85.061601
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1937.


1997KA10      Phys.Rev. C55, 640 (1997)

N.I.Kaloskamis, A.Garcia, S.E.Darden, E.Miller, W.Haeberli, P.A.Quin, B.P.Schwartz, E.Yacoub, E.G.Adelberger

Isospin Mixing in 37K and Spin Decomposition of Gamow-Teller Strength in 37Ca Decay

NUCLEAR REACTIONS 36Ar(polarized p, p), E=3.22-5.98 MeV; measured σ(θ), analyzing power vs θ vs E. 37K deduced resonances, J, π, Γ, Γp, isospin-mixing matrix elements.

RADIOACTIVITY 37Ca(β+); analyzed data; deduced Gamow-Teller transition strength related features.

doi: 10.1103/PhysRevC.55.640
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0162.


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Note: The following list of authors and aliases matches the search parameter E.Miller: , E.H.MILLER, E.K.MILLER