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NSR database version of April 27, 2024.

Search: Author = A.K.Anthony

Found 4 matches.

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2023AY06      Eur.Phys.J. A 59, 294 (2023)

Y.Ayyad, A.K.Anthony, D.Bazin, J.Chen, G.W.McCann, W.Mittig, B.P.Kay, D.K.Sharp, J.C.Zamora

Kinematics reconstruction in solenoidal spectrometers operated in active target mode

NUCLEAR REACTIONS ²H(¹⁰Be, ¹⁰Be'), E=9 MeV/nucleon; ¹H(¹⁴C, p), (¹⁴C, p'), (¹⁴C, d), E=12 MeV/nucleon; measured reaction products; deduced yields. The Active Target Time Projection Chamber (AT-TPC) of the Facility for Rare Isotope (FRIB) of the Michigan State University (MSU).

doi: 10.1140/epja/s10050-023-01205-2
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2023DR01      Phys.Rev. C 107, 034306 (2023)

N.Dronchi, D.Weisshaar, B.A.Brown, A.Gade, R.J.Charity, L.G.Sobotka, K.W.Brown, W.Reviol, D.Bazin, P.J.Farris, A.M.Hill, J.Li, B.Longfellow, D.Rhodes, S.N.Paneru, S.A.Gillespie, A.Anthony, E.Rubino, S.Biswas

Measurement of the B(E2 ↑) strengths of ³⁶Ca and ³⁸Ca

NUCLEAR REACTIONS ¹⁹⁷Au(³⁶Ca, ³⁶Ca), E=76.9 MeV/nucleon; ¹⁹⁷Au(³⁸Ca, ³⁸Ca), E=69.1 MeV/nucleon; ¹⁹⁷Au(³⁴Ar, ³⁴Ar), E not given; measured reaction products, Eγ, Iγ; deduced σ and B(E2) for the excitation of the first 2⁺ (³⁴Ar was present as contamination). ³⁶Ca; deduced proton decay branching ratio for 2 state proton unbound state, spectroscopic factors, charge radii difference with mirror nuclei ³⁶S. ³⁵K(p, γ), T=0.5-2 GK; deduced reaction rate using obtained in this paper values for the ³⁶Ca B(E2) and proton branching ratio. GRETINA HPGe array and the S800 spectrograph used to measure the γ-decay following Coulomb excitation. CAESAR CsI(Na) array and the S800 spectrograph used to measure the p/γ- branching ratio in ³⁶Ca. Systematics of first 2⁺ states energy and B(E2) for Ca isotopes. Beam produced from fragmentation reaction ⁹Be(⁴⁰Ca, X), E=140 MeV/nucleon at Coupled Cyclotron Facility (NSCL).

NUCLEAR STRUCTURE ^{36,38,40,42,44,46,48,50}Ca, ³⁶S, ³⁸Ar; calculated energy of first 2⁺ state, B(E2) for the excitation of first 2⁺ state. Shell model calculations with ZBM2, USDB, spdfu-mix and GXPF1A interactions. Comparison to experimental data.

doi: 10.1103/PhysRevC.107.034306
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Data from this article have been entered in the XUNDL database. For more information, click here.

2022GI04      Phys.Rev. C 105, 044321 (2022)

S.A.Gillespie, K.W.Brown, R.J.Charity, L.G.Sobotka, A.K.Anthony, J.Barney, A.Bonaccorso, B.A.Brown, J.Crosby, D.Dell'Aquila, J.Elson, J.Estee, A.Gade, M.Ghazali, G.Jhang, Y.Jin, B.Longfellow, W.G.Lynch, J.Pereira, M.Spieker, S.Sweany, F.C.E.Teh, A.Thomas, M.B.Tsang, C.Y.Tsang, D.Weisshaar, H.Y.Wu, K.Zhu

Proton decay spectroscopy of ²⁸S and ³⁰Cl

NUCLEAR REACTIONS ⁹Be(²⁹S, n), (³¹Ar, p), E=150 MeV/nucleon; measured reaction products, Ep, Ip, Eγ, Iγ, (particle)p-coin, pγ-coin; deduced invariant mass, momentum distribution. Setup consisting of S800 spectrograph, Si-CsI(Tl) DSSD array of 128 concentric rings and 128 annular sectors, CAESAR CsI(Na) photon detection array, BC-400-type scintillation fiber detector at A1900 fragment separator (NSCL).

RADIOACTIVITY ²⁸S(p), (2p) [from ⁹Be(²⁹S, n), E=150 MeV/nucleon]; ³⁰Cl(p), (2p) [from ⁹Be(²⁹S, n), E=150 MeV/nucleon]; measured Ep, Ip, Eγ, Iγ, pγ-coin; deduced total decay kinetic energy, decay energy spectrum. ³⁰Cl; deduced levels, J, π, S(p). ²⁸S; deduced levels, J, π, spectroscopic factors. Comparison to previous experimental results and shell model calculations.

doi: 10.1103/PhysRevC.105.044321
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Data from this article have been entered in the XUNDL database. For more information, click here.

2021JI15      Phys.Rev.Lett. 127, 262502 (2021)

Y.Jin, C.Y.Niu, K.W.Brown, Z.H.Li, H.Hua, A.K.Anthony, J.Barney, R.J.Charity, J.Crosby, D.Dell'Aquila, J.M.Elson, J.Estee, M.Ghazali, G.Jhang, J.G.Li, W.G.Lynch, N.Michel, L.G.Sobotka, S.Sweany, F.C.E.Teh, A.Thomas, C.Y.Tsang, M.B.Tsang, S.M.Wang, H.Y.Wu, C.X.Yuan, K.Zhu

First Observation of the Four-Proton Unbound Nucleus ¹⁸Mg

RADIOACTIVITY ¹⁸Mg(¹⁴O), (2p), (4p) [from ⁹Be(²⁰Mg, X)¹⁸Mg, E=170 MeV/nucleon]; measured decay products, Ep, Ip, ¹⁸Mg, ¹⁶Ne; deduced decay energy spectra, level scheme, J, π, resonance parameters. Comparison with the Gamow shell model (GSM) calculations.

doi: 10.1103/PhysRevLett.127.262502
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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 A.K.Anthony: , A.K.ANTHONY