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NSR database version of April 27, 2024.

Search: Author = T.Anderson

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2022VA04      Phys.Rev. C 105, 055802 (2022)

B.Vande Kolk, K.T.Macon, R.J.deBoer, T.Anderson, A.Boeltzig, K.Brandenburg, C.R.Brune, Y.Chen, A.M.Clark, T.Danley, B.Frentz, R.Giri, J.Gorres, M.Hall, S.L.Henderson, E.Holmbeck, K.B.Howard, D.Jacobs, J.Lai, Q.Liu, J.Long, K.Manukyan, T.Massey, M.Moran, L.Morales, D.Odell, P.O'Malley, S.N.Paneru, A.Richard, D.Schneider, M.Skulski, N.Sensharma, C.Seymour, G.Seymour, D.Soltesz, S.Strauss, A.Voinov, L.Wustrich, M.Wiescher

Investigation of the ¹⁰B (p, α)⁷Be reaction from 0.8 to 2.0 MeV

NUCLEAR REACTIONS ¹⁰B(p, α), (p, p), E=0.8-2.0 MeV; measured Eα, Iα, Ep, Ip; deduced σ(θ), σ(E) S-factor, resonance parameters of ¹⁰B+p system - energy, spin, partial (p₀, α₀, α₁) and total width. ¹⁰B(p, γ), E=0 .1-2.0 MeV; deduced σ(θ). ¹¹C; deduced levels, J, π. R-matrix analysis. Measurements were made at the University of Notre Dame (UND) Nuclear Science Laboratory (NSL) using a degrader foil method, while those at the Edwards AcceleratorLaboratory at Ohio University (OU) were performed using the time-of-flight (ToF)technique. Comparison with other experimental data.

doi: 10.1103/PhysRevC.105.055802
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2767. Data from this article have been entered in the XUNDL database. For more information, click here.

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 T_1/2 values for 2νββ and 0νββ decay modes.

doi: 10.1103/PhysRevC.104.065501
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2021MC02      Nucl.Instrum.Methods Phys.Res. B493, 15 (2021)

S.R.McGuinness, S.J.Ferran, J.T.Wilkinson, C.S.Loveless, T.Anderson, D.Blankstein, A.M.Clark, S.L.Henderson, A.D.Nelson, C.S.Reingold, M.Skulski, S.E.Lapi, G.F.Peaslee

Production of ⁵²Fe from symmetric complete fusion-evaporation reactions

NUCLEAR REACTIONS ²⁷Al(²⁸Si, 2np)⁵²Fe, E=85.5 MeV; measured reaction products, Eγ, Iγ; deduced yields, σ. Comparison with PACE4 calculations.

doi: 10.1016/j.nimb.2021.02.008
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2020AN02      Phys.Rev. C 101, 025801 (2020)

T.Anderson, M.Skulski, L.Callahan, A.Clark, A.Nelson, P.Collon, G.Chmiel, T.Woodruff, M.Caffee

Measurement of ³⁴S(³He, p)³⁶Cl cross sections for nuclide enrichment in the early solar system

NUCLEAR REACTIONS ³He(³⁴S, p)³⁶Cl, E=1.11-2.36 MeV/nucleon; measured production σ(E) for ³⁶Cl at NSL, University of Notre Dame, ³⁶Cl atoms by accelerator mass spectroscopy (AMS) at NSL and at PRIME laboratory, Purdue University. Comparison with predictions from TALYS and other models. Discussed astrophysical implications of ³⁶Cl in terms of presence of short-lived radionuclides (SLRs) at the time of the formation of the solar system.

doi: 10.1103/PhysRevC.101.025801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2455.

2020GU11      Phys.Lett. B 806, 135473 (2020)

Y.K.Gupta, B.K.Nayak, U.Garg, K.Hagino, K.B.Howard, N.Sensharma, M.Senyigit, W.P.Tan, P.D.O'Malley, M.Smith, R.Gandhi, T.Anderson, R.J.deBoer, B.Frentz, A.Gyurjinyan, O.Hall, M.R.Hall, J.Hu, E.Lamere, Q.Liu, A.Long, W.Lu, S.Lyons, K.Ostdiek, C.Seymour, M.Skulski, B.Vande Kolk

Determination of hexadecapole (β₄) deformation of the light-mass nucleus ²⁴Mg using quasi-elastic scattering measurements

NUCLEAR REACTIONS ⁹⁰Zr(¹⁶O, ¹⁶O), (²⁴Mg, ²⁴Mg), E=61 MeV; measured reaction products. ²⁴Mg; deduced deformation parameters, σ, B(Eλ). CCFULL calculations.

doi: 10.1016/j.physletb.2020.135473
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Data from this article have been entered in the XUNDL database. For more information, click here.

2019RE04      Eur.Phys.J. A 55, 77 (2019)

C.S.Reingold, O.Olivas-Gomez, A.Simon, J.Arroyo, M.Chamberlain, J.Wurzer, A.Spyrou, F.Naqvi, A.C.Dombos, A.Palmisano, T.Anderson, A.M.Clark, B.Frentz, M.R.Hall, S.L.Henderson, S.Moylan, D.Robertson, M.Skulski, E.Stech, S.Y.Strauss, W.P.Tan, B.Vande Kolk

High Efficiency Total Absorption Spectrometer HECTOR for capture reaction measurements

RADIOACTIVITY ⁶⁰Co(IT); measured Eγ, Iγ using Total Absorption Spectrometer HECTOR; deduced sum spectrum; compared with GEANT4 simulated spectrum.

NUCLEAR REACTIONS ²⁷Al(p, γ), E not given; measured Eγ, Iγ; deduced resonances, average multiplicities, summing efficiencies and resonance strengths; compared with GEANT4 simulations and with published data. Remark: Paper aimed mainly to show the possibilities of the HECTOR spectrometer.

doi: 10.1140/epja/i2019-12748-8
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Data from this article have been entered in the XUNDL database. For more information, click here.

2017AN08      Phys.Rev. C 96, 015803 (2017)

T.Anderson, M.Skulski, A.Clark, A.Nelson, K.Ostdiek, P.Collon, G.Chmiel, T.Woodruff, M.Caffee

Re-measurement of the ³³S (α, p)³⁶Cl cross section for early solar system nuclide enrichment

NUCLEAR REACTIONS ⁴He(³³S, ³⁶Cl), E=0.78-1.52 MeV/nucleon; measured ³⁶Cl/Cl concentrations by AMS technique, integrated σ(E) at the Tandem accelerator of the NSL, University of Notre Dame. Comparison with previous experimental measurements and with Hauser-Feshbach code TALYS. Systematically lower cross sections obtained in the present work than in the originally reported ones, thus resolving the discrepancy with theoretical calculations.

doi: 10.1103/PhysRevC.96.015803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2268.

2017OS02      Phys.Rev. C 95, 055809 (2017)

K.M.Ostdiek, T.S.Anderson, W.K.Bauder, M.R.Bowers, A.M.Clark, P.Collon, W.Lu, A.D.Nelson, D.Robertson, M.Skulski, R.Dressler, D.Schumann, J.P.Greene, W.Kutschera, M.Paul

Activity measurement of ⁶⁰Fe through the decay of ^60mCo and confirmation of its half-life

RADIOACTIVITY ⁶⁰Fe(β^-)[from Cu(p, X), E=590 MeV at PSI followed by chemical separation]; ^60mCo(IT); measured Eγ, Iγ from ^60mCo decay, half-life of ⁶⁰Fe via the 2+ isomeric state of ⁶⁰Co, number of atoms of ⁶⁰Fe from ⁶⁰Fe/⁵⁶Fe isotopic ratios of samples using accelerator mass spectrometry (AMS) technique. Experiments performed at the university of Notre Dame. Comparison with previous half-life measurements.

doi: 10.1103/PhysRevC.95.055809
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Data from this article have been entered in the XUNDL database. For more information, click here.

2015OS02      Nucl.Instrum.Methods Phys.Res. B361, 638 (2015)

K.Ostdiek, T.Anderson, W.Bauder, M.Bowers, P.Collon, R.Dressler, J.Greene, W.Kutschera, W.Lu, M.Paul, D.Robertson, D.Schumann, M.Skulski, A.Wallner

Towards a measurement of the half-life of ⁶⁰Fe for stellar and early Solar System models

RADIOACTIVITY ⁶⁰Fe(β^-); measured decay products; deduced T_1/2. Accelerator mass spectrometry, comparison with available data.

doi: 10.1016/j.nimb.2015.05.033
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Data from this article have been entered in the XUNDL database. For more information, click here.

2012CO16      Phys.Rev. C 86, 015809 (2012)

A.L.Cole, T.S.Anderson, R.G.T.Zegers, S.M.Austin, B.A.Brown, L.Valdez, S.Gupta, G.W.Hitt, O.Fawwaz

Gamow-Teller strengths and electron-capture rates for pf-shell nuclei of relevance for late stellar evolution

NUCLEAR REACTIONS ⁴⁵Sc, ⁴⁸Ti, ⁵¹V, ^54,56Fe, ⁵⁵Mn, ⁵⁹Co, ^58,60,62,64Ni(n, p), E GE 100 MeV/nucleon; ⁴⁸Ti, ^50,51V, ^58,64Ni, ⁶⁴Zn(d, ²He), E GE 100 MeV/nucleon; ⁵⁸Ni, ⁶⁴Zn(t, ³He), E GE 100 MeV/nucleon; ^60,62Ni(p, n), E GE 100 MeV/nucleon; calculated B(GT) distributions, and electron capture (EC) rates at relevant stellar temperatures and densities using shell-model with GXPF1a and KB3G effective interactions, and QRPA using ground-state deformation parameters and masses from the finite-range droplet model. Comparison with experimental data. Relevance to late stellar evolution.

RADIOACTIVITY ⁴⁵Ca, ⁵⁵Cr, ⁶⁴Co, ⁶⁴Cu(β^-); calculated B(GT) strength distribution, EC rates using shell-model and QRPA. Comparison with experimental data.

doi: 10.1103/PhysRevC.86.015809
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2005FI10      Phys.Rev. C 72, 024321 (2005)

S.M.Fischer, T.Anderson, P.Kerns, G.Mesoloras, D.Svelnys, C.J.Lister, D.P.Balamuth, P.A.Hausladen, D.G.Sarantites

Shape coexistence in ⁷¹Br and the question of the ground-state spin of ⁷¹Kr

NUCLEAR REACTIONS ⁴⁰Ca(⁴⁰Ca, p2α), E=160 MeV; measured Eγ, Iγ, γγ-, (charged particle)γ-coin. ⁷¹Br deduced levels, J, π, δ, rotational bands, shape coexistence features. ⁷¹Kr; analyzed data; deduced ground-state J, π. Gammasphere, Microball arrays.

doi: 10.1103/PhysRevC.72.024321
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Data from this article have been entered in the XUNDL database. For more information, click here.

Note: The following list of authors and aliases matches the search parameter T.Anderson: , T.J.ANDERSON, T.S.ANDERSON