Nuclear Science References (NSR)

NUCLEAR REACTIONS ^245,248Cm, ^242,244Pu, ²³⁸U, ²³²Th, ²²⁶Ra(⁴⁸Ca, n), (⁴⁸Ca, 2n), (⁴⁸Ca, 3n), (⁴⁸Ca, 4n), (⁴⁸Ca, 5n), E^*=10-70 MeV; calculated σ(E), excitation functions. Comparison to available experimental data.

doi: 10.1103/PhysRevC.106.014614
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2022HO13 Eur.Phys.J. A 58, 180 (2022)

J.Hong, G.G.Adamian, N.V.Antonenko, M.Kowal, P.Jachimowicz

Hot and cold fusion reactions leading to the same superheavy evaporation residue

NUCLEAR REACTIONS ^233,235U(⁴⁸Ca, X)²⁷⁷Cn, E not given; calculated σ; deduced the possibility of filling the gap between the isotopes of superheavy nuclei with Z=112 produced in cold and hot fusion reactions. Comparison with available data.

doi: 10.1140/epja/s10050-022-00826-3
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2021HO08 Phys.Rev. C 103, L041601 (2021)

J.Hong, G.G.Adamian, N.V.Antonenko, P.Jachimowicz, M.Kowal

Rate of decline of the production cross section of superheavy nuclei with Z = 114-117 at high excitation energies

NUCLEAR REACTIONS ^242,244Pu(⁴⁸Ca, n), (⁴⁸Ca, 2n), (⁴⁸Ca, 3n), (⁴⁸Ca, 4n), E^*=10-65 MeV; ^242,244Pu, ²⁴³Am, ²⁴⁸Cm, ²⁴⁹Bk(⁴⁸Ca, 5n), (⁴⁸Ca, 6n), (⁴⁸Ca, 7n), (⁴⁸Ca, 8n), (⁴⁸Ca, 9n), E^*=40-120 MeV; calculated σ(E) using microscopic-macroscopic (MM) method, and compared with available experimental data for superheavy nuclei (SHN).

NUCLEAR STRUCTURE ²⁹⁰Ts; calculated potential energy surface (PES) in (β₂₀, β₂₂) plane. ^{286,287,288,289,290,291,292,293,294,295,296,297,298}Fl, ^{287,288,289,290,291,292,293,294,295,296,297,298,299}Mc, ^{288,289,290,291,292,293,294,295,296,297,298,299,300}Lv, ^{289,290,291,292,293,294,295,296,297,298,299,300,301}Ts; calculated fission barriers and S(n) using microscopic-macroscopic (MM) method, and standard BCS method with blocking for nuclei with odd numbers of protons, neutrons, or both.

doi: 10.1103/PhysRevC.103.L041601
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2021HO11 Phys.Rev. C 103, 054907 (2021)

J.Hong, S.H.Lee

Energy loss of heavy quarkonia in hot QCD plasmas

doi: 10.1103/PhysRevC.103.054907
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2020HO07 Phys.Lett. B 805, 135438 (2020)

J.Hong, G.G.Adamian, N.V.Antonenko

Could new isotopes of superheavies with Z=112-118 be produced in ⁴⁸Ca-induced cold fusion reactions?

NUCLEAR REACTIONS ²³⁸U, ²³⁷Np, ^{239,240,242,244}Pu, ²⁴³Am, ^245,248Cm, ²⁴⁹Bk, ²⁴⁹Cf(⁴⁸Ca, X), E not given; calculated σ forthe production of new heaviest isotopes of the SHN with charge numbers 112-118 1-n and 2-n evaporation channels. Comparison with experimental data.

doi: 10.1016/j.physletb.2020.135438
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2020HO13 Phys.Lett. B 809, 135760 (2020)

J.Hong, G.G.Adamian, N.V.Antonenko, P.Jachimowicz, M.Kowal

Possibilities of direct production of superheavy nuclei with Z=112-118 in different evaporation channels

NUCLEAR REACTIONS ^242,244Pu, ²⁴³Am, ^245,248Cm, ²⁴⁹Bk, ^249,252Cf(⁴⁸Ca, X), E not given; analyzed available data. ^{276,277,278,279,280,281,282,283,284,285,286,287,288}Cn, ^{280,281,282,283,284,285,286,287,288,289,290,291,292}Fl, ^{286,287,288,289,290,291,292,293,294,295,296}Lv, ^{291,292,293,294,295,296,297,298,299}Og, ^{279,280,281,282,283,284,285,286,287,288,289,290,291}Nh, ^{285,286,287,288,289,290,291,292,293,294,295}Mc, ^{291,292,293,294,295,296,297,298}Ts; deduced theoretical barriers and energy thresholds n the evaporation channels with emission of proton and alpha-particle.

doi: 10.1016/j.physletb.2020.135760
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2020TA14 Phys.Rev. C 102, 021901 (2020)

H.Taya, A.Park, S.Cho, P.Gubler, K.Hattori, J.Hong, X.-G.Huang, S.H.Lee, A.Monnai, A.Ohnishi, M.Oka, D.-L.Yang, for the ExHIC-P Collaboration

Signatures of the vortical quark-gluon plasma in hadron yields

doi: 10.1103/PhysRevC.102.021901
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2019HO04 Phys.Rev. C 99, 034905 (2019)

J.Hong, S.H.Lee

Quarkonium dissociation in perturbative QCD

doi: 10.1103/PhysRevC.99.034905
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2018HO09 Phys.Rev. C 98, 014913 (2018)

J.Hong, S.Cho, T.Song, S.H.Lee

Hadronic effects on the ccq-barq-bar tetraquark state in relativistic heavy ion collisions

doi: 10.1103/PhysRevC.98.014913
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2017HO16 Phys.Rev. C 96, 014609 (2017)

J.Hong, G.G.Adamian, N.V.Antonenko

Possibilities of production of transfermium nuclei in complete fusion reactions with radioactive beams

NUCLEAR REACTIONS ²⁴⁸Cm(¹⁶C, xn)²⁵⁹No/²⁶⁰No/²⁶¹No/²⁶²No/²⁶³No, E*=10-70 MeV; ²⁴⁸Cm(¹⁶C, xnα)²⁵⁶Fm/²⁵⁷Fm/²⁵⁸Fm, E*=30-85 MeV; ²⁴⁹Bk(¹⁶C, xn)²⁶⁰Lr/²⁶¹Lr/²⁶²Lr/²⁶³Lr/²⁶⁴Lr, E*=10-70 MeV; ²⁴⁹Bk(¹⁶C, xnα)²⁵⁷Md/²⁵⁸Md/²⁵⁹Md, E*=30-85 MeV; ²⁴⁴Pu(²⁰O, xn)²⁵⁹No/²⁶⁰No/²⁶¹No/²⁶²No/²⁶³No, E*=10-70 MeV; ²⁴⁴Pu(²⁰O, xnα)²⁵⁶Fm/²⁵⁷Fm/²⁵⁸Fm, E*=30-85 MeV; ²⁴⁴Pu(²¹O, xn)²⁶⁰No/²⁶¹No/²⁶²No/²⁶³No, E*=10-70 MeV; ²⁴⁴Pu(²¹O, xnα)²⁵⁷Fm/²⁵⁸Fm/²⁵⁹Fm, E*=30-85 MeV; ²⁴⁸Cm(²⁰O, xn)²⁶³Rf/²⁶⁴Rf/²⁶⁵Rf/²⁶⁶Rf/²⁶⁷Rf, E*=10-70 MeV; ²⁴⁸Cm(²⁰O, xnα)²⁶⁰No/²⁶¹No/²⁶²No, E*=10-70 MeV; ²⁴⁸Cm(²¹O, xn)²⁶⁴Rf/²⁶⁵Rf/²⁶⁶Rf/²⁶⁷Rf, E*=10-70 MeV; ²⁴⁸Cm(²¹O, xnα)²⁶¹No/²⁶²No/²⁶³No, E*=10-70 MeV; ²³⁸U(²⁸Mg, xn)²⁶¹Rf/²⁶²Rf/²⁶³Rf, E*=25-65 MeV; ²³⁸U(²⁸Mg, xnα)²⁵⁸No/²⁵⁹No/²⁶⁰No, E*=35-75 MeV; ²⁴⁴Pu(²⁸Mg, xn)²⁶⁷Sg/²⁶⁸Sg/²⁶⁹Sg, E*=25-65 MeV; ²⁴⁴Pu(²⁸Mg, xnα)²⁶⁴Rf/²⁶⁵Rf/²⁶⁶Rf, E*=35-75 MeV; ²⁴⁴Pu(³⁰Mg, xn)²⁶⁹Sg/²⁷⁰Sg, E*=30-60 MeV; ²⁴⁴Pu(³⁰Mg, xnα)²⁶⁶Rf/²⁶⁷Rf, E*=35-75 MeV; ²⁴⁹Bk(²⁰O, xn)²⁶⁴Db/²⁶⁵Db/²⁶⁶Db/²⁶⁷Db/²⁶⁸Db, E*=10-70 MeV; ²⁴⁹Bk(²⁰O, xnα)²⁶¹Lr/²⁶²Lr/²⁶³Lr, E*=30-75 MeV; ²⁴⁹Bk(²¹O, xn)²⁶⁴Db/²⁶⁵Db/²⁶⁶Db/²⁶⁷Db/²⁶⁸Db/²⁶⁹Db, E*=10-70 MeV; ²⁴⁹Bk(²¹O, xnα)²⁶²Lr/²⁶³Lr/²⁶⁴Lr, E*=30-75 MeV; ²⁴⁸Cm(²¹F, xn)²⁶⁴Db/²⁶⁵Db/²⁶⁶Db/²⁶⁷Db, E*=10-70 MeV; ²⁴⁸Cm(²¹F, xnα)²⁶¹Lr/²⁶²Lr/²⁶³Lr, E*=30-75 MeV; ²⁴⁸Cm(²³F, xn)²⁶⁶Db/²⁶⁷Db/²⁶⁸Db/²⁶⁹Db/²⁷⁰Db, E*=10-70 MeV; ²⁴⁸Cm(²³F, xnα)²⁶³Lr/²⁶⁴Lr/²⁶⁵Lr, E*=30-75 MeV; ²⁴⁴Pu(²⁴Na, xn)²⁶³Db/²⁶⁴Db, E*=35-60 MeV; ²⁴⁴Pu(²⁴Na, xnα)²⁶⁰Lr/²⁶¹Lr, E*=40-75 MeV; ²⁴⁴Pu(²⁵Na, xn)²⁶⁴Db/²⁶⁵Db/²⁶⁶Db/²⁶⁷Db, E*=15-65 MeV; ²⁴⁴Pu(²⁵Na, xnα)²⁶¹Lr/²⁶²Lr/²⁶³Lr, E*=35-75 MeV; ²⁴⁴Pu(²⁷Na, xn)²⁶⁶Db/²⁶⁷Db/²⁶⁸Db/²⁶⁹Db, E*=15-65 MeV; ²⁴⁴Pu(²⁷Na, xnα)²⁶³Lr/²⁶⁴Lr/²⁶⁵Lr, E*=30-75 MeV; ²⁵¹Cf(²⁰O, xn)²⁶⁶Sg/²⁶⁷Sg/²⁶⁸Sg/²⁶⁹Sg, E*=15-60 MeV; ²⁵¹Cf(²⁰O, xnα)²⁶³Rf/²⁶⁴Rf/²⁶⁵Rf, E*=30-75 MeV; ²⁵¹Cf(²¹O, xn)²⁶⁷Sg/²⁶⁸Sg/²⁶⁹Sg/²⁷⁰Sg, E*=15-60 MeV; ²⁵¹Cf(²¹O, xnα)²⁶⁴Rf/²⁶⁵Rf/²⁶⁶Rf, E*=30-75 MeV; ²⁴⁹Cf(²¹O, xn)²⁶⁵Sg/²⁶⁶Sg/²⁶⁷Sg/²⁶⁸Sg, E*=15-60 MeV; ²⁴⁹Cf(²¹O, xnα)²⁶²Rf/²⁶³Rf/²⁶⁴Rf, E*=30-75 MeV; ²⁵⁰Cf(²¹O, xn)²⁶⁶Sg/²⁶⁷Sg/²⁶⁸Sg/²⁶⁹Sg, E*=15-60 MeV; ²⁵⁰Cf(²¹O, xnα)²⁶³Rf/²⁶⁴Rf/²⁶⁵Rf, E*=30-75 MeV; ²⁴⁸Cm(²⁴Ne, xn)²⁶⁷Sg/²⁶⁸Sg/²⁶⁹Sg/²⁷⁰Sg, E*=15-65 MeV; ²⁴⁸Cm(²⁴Ne, xnα)²⁶⁴Rf/²⁶⁵Rf/²⁶⁶Rf, E*=30-75 MeV; ²⁴⁸Cm(²⁵Ne, xn)²⁶⁸Sg/²⁶⁹Sg/²⁷⁰Sg/²⁷¹Sg, E*=15-65 MeV; ²⁴⁸Cm(²⁵Ne, xnα)²⁶⁵Rf/²⁶⁶Rf/²⁶⁷Rf, E*=30-75 MeV; ²⁴⁸Cm(²⁶Ne, xn)²⁶⁹Sg/²⁷⁰Sg/²⁷¹Sg/²⁷²Sg, E*=15-65 MeV; ²⁴⁸Cm(²⁶Ne, xnα)²⁶⁶Rf/²⁶⁷Rf/²⁶⁸Rf, E*=30-75 MeV; calculated σ(E*) for xn and αxn reactions in various asymmetric hot fusion-evaporation reactions with radioactive beams, and compared with available experimental data. ²⁴⁸Cm(¹⁶C, 3n), E*=29.2 MeV; ²⁴⁸Cm(²⁰O, 3nα), E*=48.3 MeV; ²⁴⁸Cm(²¹O, 4nα), E*=54.4 MeV; ²⁴⁸Cm(¹⁶C, n), E*=11.8 MeV; ²⁴⁴Pu(²⁰O, n), E*=11.8 MeV; ²⁴⁴Pu(²¹O, 2n), E*=18.3 MeV; ²⁴⁴Pu(²¹O, n), E*=12.1 MeV; ²⁴⁹Bk(¹⁶C, 2n), E*=17.7 MeV; ²⁴⁹Bk(²¹O, 3nα), E*=44.8 MeV; ²⁴⁸Cm(²³F, 4nα), E*=50.5 MeV; ²⁴⁴Pu(²⁷Na, 4nα), E*=50.9 MeV; ²⁴⁹Bk(²¹O, 2nα), E*=40.8 MeV; ²⁴⁸Cm(²³F, 3nα), E*=46.1 MeV; ²⁴⁴Pu(²⁷Na, 3nα), E*=47.0 MeV; ²⁴⁸Cm(²³F, 2nα), E*=40.8 MeV; ²⁴⁴Pu(²⁷Na, 2nα), E*=42.1 MeV; ²⁴⁸Cm(²⁰O, 5n), E*=46.4 MeV; ²⁴⁸Cm(²⁰O, 4n), E*=38.7 MeV; ²⁴⁸Cm(²¹O, 5n), E*=43.6 MeV; ²⁴⁸Cm(²⁰O, 2n), E*=17.7 MeV; ²⁴⁸Cm(²¹O, 3n), E*=24.6 MeV; ²⁴⁸Cm(²⁵Ne, 3nα), E*=44.3 MeV; ²⁴⁸Cm(²⁶Ne, 4nα), E*=50.5 MeV; ²⁴⁴Pu(³⁰Mg, 4nα), E*=50.9 MeV; ²⁴⁸Cm(²¹O, n), E*=10.7 MeV; ²⁴⁸Cm(²⁶Ne, 2nα), E*=40.4 MeV; ²⁴⁹Bk(²⁰O, 5n), E*=45.9 MeV; ²⁴⁸Cm(²¹F, 5n), E*=48.2 MeV; ²⁴⁴Pu(²⁵Na, 5n), E*=48.9 MeV; ²⁴⁹Bk(²⁰O, 4n), E*=37.9 MeV; ²⁴⁹Bk(²¹O, 5n), E*=43.3 MeV; ²⁴⁸Cm(²¹F, 4n), E*=38.9 MeV; ²⁴⁸Cm(²³F, 2n), E*=17.2 MeV; ²⁵¹Cf(²⁰O, 4n), E*=40.3 MeV; ²⁴⁹Cf(²¹O, 5n), E*=49.6 MeV; ²⁵⁰Cf(²¹O, 4n), E*=40.3 MeV; ²⁵¹Cf(²¹O, 3n), E*=28.7 MeV; ²⁴⁸Cm(²⁴Ne, 5n), E*=46.2 MeV; ²⁴⁹Cf(²¹O, 4n), E*=41.8 MeV; ²⁴⁸Cm(²⁴Ne, 4n), E*=38.2 MeV; ²⁴⁸Cm(²⁵Ne, 5n), E*=43.1 MeV; ²⁴⁸Cm(²⁶Ne, 4n), E*=37.9 MeV; ²⁴⁴Pu(³⁰Mg, 4n), E*=37.6 MeV; ²⁴⁸Cm(²⁶Ne, 2n), E*=17.3 MeV; calculated evaporation residue cross sections. Dinuclear system (DNS) model.

doi: 10.1103/PhysRevC.96.014609
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2017HO27 Phys.Rev. C 96, 064603 (2017)

J.Hong, C.A.Bertulani, A.T.Kruppa

Neutron removal from the deformed halo nucleus ³¹Ne

NUCLEAR REACTIONS ¹²C(³¹Ne, ³⁰Ne), E=230 MeV/nucleon; calculated neutron knockout cross sections and longitudinal momentum distributions as function of deformation using a model to include deformed wave functions and a dynamical knockout formalism that includes the dependence on the nuclear orientation to study the neutron removal. Comparison with experimental data. ³¹Ne; deduced 3/2- for the deformed halo nucleus.

doi: 10.1103/PhysRevC.96.064603
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2017TS02 Phys.Rev. C 95, 044614 (2017)

M.B.Tsang, J.Estee, H.Setiawan, W.G.Lynch, J.Barney, M.B.Chen, G.Cerizza, P.Danielewicz, J.Hong, P.Morfouace, R.Shane, S.Tangwancharoen, K.Zhu, T.Isobe, M.Kurata-Nishimura, J.Lukasik, T.Murakami, Z.Chajecki, for the S|pRIT Collaboration

Pion production in rare-isotope collisions

NUCLEAR REACTIONS ¹³²Sn(¹²⁴Sn, X), ¹⁰⁸Sn(¹¹²Sn, X), E=300, 200 MeV/nucleon; calculated center-of-mass energy spectra for neutrons, protons, tritons, ³He, π^- and π⁺ particles emitted in central collisions, comparison of π^-/π⁺ spectral and isoscaling ratios in the two reactions, pion energy spectra. Simulations used the Boltzmann-Uehling-Uhlenbeck transport model.

doi: 10.1103/PhysRevC.95.044614
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2016HO19 Phys.Rev. C 94, 044606 (2016)

J.Hong, G.G.Adamian, N.V.Antonenko

Possibilities of production of transfermium nuclei in charged-particle evaporation channels

NUCLEAR REACTIONS ²³⁸U(¹²C, 4n), E(cm)=64.3 MeV; ²³⁸U(¹²C, 5n), E(cm)=70.0 MeV; ²³⁸U(¹²C, 6n), E(cm)=79.5 MeV; ²³⁸U(¹²C, 7n), E(cm)=90.4 MeV; ²³⁸U(¹²C, 8n), E(cm)=109.5 MeV; ²⁴⁰Pu(¹²C, 4n), E(cm)=67.6 MeV; ²³³U(¹⁶O, 4n), E(cm)=87.0 MeV; ²³³U(¹⁶O, 5n), E(cm)=90.8 MeV; ²³²Th(²⁰Ne, 5n), E(cm)=107.8 MeV; ²³²Th(²⁰Ne, 6n), E(cm)=111.4 MeV; ²³²Th(²²Ne, 7n), E(cm)=121.2 MeV; ²³²Th(²²Ne, 8n), E(cm)=129.4 MeV; ²⁴⁸Cm(¹⁵N, 4n), E(cm)=76.4 MeV; ²⁴⁸Cm(¹⁵N, 5n), E(cm)=82.0 MeV; ²³²Th(²⁷Al, 5n), (²⁷Al, 6n), E(cm)=136.0 MeV; ²⁴⁹Bk(¹⁵N, 4n), E(cm)=75.5 MeV; ²⁴²Pu(²²Ne, 4n), E(cm)=104.9 MeV; ²⁴⁴Pu(²²Ne, 4n), (²²Ne, 5n), E(cm)=104.9 MeV; ²⁴⁹Bk(¹⁸O, 4n), E(cm)=86.7 MeV; ²⁴⁹Bk(¹⁸O, 5n), E(cm)=92.3 MeV; ²⁴⁸Cm(¹⁹F, 5n), E(cm)=95.8 MeV; ²⁴¹Am(²²Ne, 4n), E(cm)=108.1 MeV; ²⁴³Am(²²Ne, 4n), E(cm)=106.4 MeV; ²³⁶U(²⁷Al, 5n), E(cm)=138.2 MeV; ²³⁶U(²⁷Al, 6n), E(cm)=146.3 MeV; ²³²Th(³¹P, 5n), E(cm)=151.4 MeV; ²⁴⁹Cf(¹⁸O, 4n), E(cm)=88.6 MeV; ²³⁸U(³⁰Si, 4n), E(cm)=133.0 MeV; ²³⁸U(³⁰Si, 5n), E(cm)=144.0 MeV; ²⁴⁹Bk(²²Ne, 4n), (²²Ne, 5n), E(cm)=113.0 MeV; calculated evaporation residue σ, and compared with available experimental data. ²⁴²Pu(¹²C, 4n), (¹²C, 4nα), (¹²C, 5nα), (¹⁸O, 4n), (¹⁸O, 5n), (¹⁸O, 3np), (²²Ne, 2np), (³⁰Si, nα), (³⁰Si, 2nα), (³⁰Si, 2np), (³⁰Si, 3np), (³⁶S, 2nα), (³⁶S, 3nα), (³⁶S, 4nα), ²³⁸U(¹⁶O, 4n), (¹⁶O, 5n), (¹⁶O, 6n), (¹⁶O, 4nα), (¹⁶O, 5nα), (²²Ne, 4n), (²²Ne, 5n), (²²Ne, 6n), (²²Ne, 2np), (²²Ne, 3np), (²²Ne, 4np), (²²Ne, nα), (²²Ne, 2nα), (²²Ne, 3nα), (²²Ne, 4nα), (³⁰Si, 2np), (³⁰Si, 3np), (³⁶S, nα), (³⁶S, 2nα), (³⁶S, 3nα), (³⁶S, 4nα), (³⁶S, 3np), ²⁴⁸Cm(¹⁸O, 4n), (¹⁸O, 5n), (¹⁸O, 6n), (¹⁸O, nα), (¹⁸O, 2nα), (¹⁸O, 3nα), (¹⁸O, np), (¹⁸O, 2np), (¹⁸O, 3np), (¹⁸O, 4np), (¹⁹F, nα), (¹⁹F, 2nα), (¹⁹F, 2np), (²²Ne, 5n), (²²Ne, 2np), (²²Ne, 3np), (²²Ne, 4np), (²²Ne, 5np), (²²Ne, nα), (²²Ne, 2nα), (²²Ne, 3nα), (²²Ne, 4nα), (¹⁵N, np), (¹⁵N, 2np), (²⁶Mg, npα), (²⁶Mg, 2npα), (²⁶Mg, 3npα), (²⁶Mg, 4npα), (²⁶Mg, nα), (²⁶Mg, 2nα), (²⁶Mg, 3nα), (²⁶Mg, 4nα), (²⁶Mg, 2np), (²⁶Mg, 3np), (²⁶Mg, 4np), (²⁷Al, 2nα), (²⁷Al, 3nα), (²⁷Al, 4nα), (²⁷Al, 5nα), (³⁰Si, 2nα), (³⁰Si, 3nα), (³⁰Si, 4nα), (³⁰Si, 5nα), (³¹P, 2nα), (³¹P, 3nα), (³¹P, 4nα), ²⁴⁹Cf(¹⁵N, 4n), (¹⁵N, 2nα), (¹⁵N, 3nα), (¹⁸O, np), (¹⁸O, 2np), ²⁰⁸Pb(⁴⁸Ca, np), (⁴⁸Ca, 2np), (⁴⁸Ca, 3np), (⁴⁸Ca, 4np), (⁴⁸Ca, nα), (⁴⁸Ca, 2nα), (⁴⁸Ca, 3nα), (⁴⁸Ca, 4nα), ²³⁴U(²²Ne, np), (²²Ne, 2np), (²²Ne, 3np), (²²Ne, 4np), (²²Ne, nα), (²²Ne, 2nα), (²²Ne, 3nα), (²²Ne, 4nα), ²³⁸U(²²Ne, 2np), (²²Ne, 3np), (²²Ne, 4np), (²²Ne, nα), (²²Ne, 2nα), (²²Ne, 3nα), (²²Ne, 4nα), ²³⁴U(²²Ne, np), (³⁰Si, 2np), (³⁰Si, 3np), (³⁶S, nα), (³⁶S, 2nα), (³⁶S, 3nα), (³⁶S, 4nα), (³⁶S, 3np), ²⁴⁴Pu(¹⁸P, np), (¹⁸P, 2np), (¹⁹F, 2np), (²²Ne, nα), (²²Ne, 2nα), (²²Ne, 2np), (²²Ne, 3np), (²²Ne, 4np), (²³Na, 2nα), (²⁶Mg, nα), (²⁶Mg, 2nα), (²⁶Mg, 2np), (²⁶Mg, 3np), (²⁶Mg, 4np), (²⁶Mg, 5np), ²⁴⁹Bk(¹⁵N, np), (¹⁵N, 2np), (¹⁸O, nα), (¹⁸O, 2nα), (¹⁸O, np), (¹⁸O, 2np), (²²Ne, nα), (²²Ne, 2nα), (²²Ne, 3nα), (²²Ne, 2np), (²²Ne, 3np), (²²Ne, 4np), (²⁶Mg, 2α), (²⁶Mg, n2α), (²⁶Mg, 2n2α), (²⁶Mg, nα), (²⁶Mg, 2nα), (²⁶Mg, 3nα), (²⁶Mg, 4nα), (²⁶Mg, 5nα), (²⁷Al, 2nα), (²⁷Al, 3nα), (²⁷Al, 4nα), (³⁰Si, nα), (³⁰Si, 2nα), (³⁰Si, 3nα), (³⁰Si, 4nα), (³⁰Si, 5nα), ²³⁵U(³⁶S, nα), (³⁶S, 2np), ²³³U(³⁶S, 2np), ²⁴⁵Cm(³⁰Si, nα), (³⁰Si, 2nα), (³⁰Si, 3nα), (³⁰Si, 4nα), ²⁴⁰Pu(³⁶S, nα), (³⁶S, 2nα), (³⁶S, 3nα), (³⁶S, 4nα), E*=20-90 MeV; calculated production σ(E_CN) in xn, pxn, αxn channels using dinuclear system (DNS) model, and compared with available experimental data. ^259,260Md, ^260,261No, ^{261,262,263,264}Lr, ^264,265Rf, ^{264,265,266,267,268}Db, ^{266,267,268,269}Sg, ^{267,268,269,270,271}Bh, ^{267,268,269,270,271,272,273,274}Hs, ^{270,271,272,273,274}Mt; calculated production σ in pxn and αxn evaporation channels of the asymmetric hot fusion reactions. Comparison with available experimental data.

doi: 10.1103/PhysRevC.94.044606
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2016HO22 Eur.Phys.J. A 52, 305 (2016)

J.Hong, G.G.Adamian, N.V.Antonenko

Possibilities of synthesis of unknown isotopes of superheavy nuclei with charge numbers Z > 108 in asymmetric actinide-based complete fusion reactions

NUCLEAR REACTIONS ²³²Th(²⁷Al, xn), (³¹P, xn), E^*≈25-70 MeV;^233,235,238U(²⁸Si, xn), (²⁹Si, xn), (³⁰Si, xn), E^*≈25-70 MeV;²³⁵U(³⁶S, 3n), E^*=29-47 MeV;²³⁷Np(³⁶S, 4n), E^*=35-61 MeV;²³⁷Np(³⁴S, 4n), E^*=40-59 MeV;²⁴⁰Pu(³⁶S, 3n), E^*=26-51 MeV;²⁴⁰Pu(³⁶S, 4n), E^*=36-56 MeV;²⁴²Pu(³⁰Si, 4n), E^*=39-57 MeV;²⁴²Pu(³⁶S, 3n), E^*=28-49 MeV;²⁴²Pu(³⁶S, 4n), E^*=34-55 MeV;²⁴²Pu(³⁶S, 5n), E^*=44-60 MeV;²⁴⁴Pu(²⁹Si, 5n), E^*=50-61 MeV;²⁴¹Am(³⁴S, 4n), E^*=41-53 MeV;²⁴¹Am(³⁶S, 3n), E^*=28-45 MeV;²⁴¹Am(³⁶S, 4n), E^*=36-53 MeV;²⁴⁵Cm(³⁶S, 2nα), E^*=36-54 MeV;²⁴⁵Cm(³⁶S, 3nα), E^*=42-64 MeV;²⁴⁸Cm(¹⁵N, xn), (¹⁹F, xn), E^*≈25-65 MeV;(²⁷Al, 3n), E^*=28-39 MeV;²⁴⁸Cm(²⁷Al, 4n), E^*=36-58 MeV;²⁴⁹Bk(¹⁵N, xn), (¹⁸O, xn), (²²Ne, xn);E^*≈25-63 MeV;²⁴⁹Bk(²⁶Mg, 3n), E=26-45 MeV;²⁴⁹Bk(²⁶Mg, 4n), E^*=34-54 MeV;²⁴⁹Cf(¹⁸O, xn), E^*=25-62 MeV[x=3-5 for all nuclei];²⁴⁹Cf(³⁰Si, 3n), E^*=29-49 MeV;²⁴⁹Cf(³⁰Si, 4n), E^*=39-57 MeV;²⁴⁹Cf(³⁶S, 2n), E^*=20-36 MeV;²⁴⁹Cf(³⁶S, 3n), E^*=29-49 MeV;²⁴⁹Cf(³⁶S, 4n), E^*=40-53 MeV;²⁴⁹Cf(³⁰Si, nα), E^*=26-49 MeV;²⁴⁹Cf(³⁰Si, 3nα), E^*=42-68 MeV; calculated evaporation residue σ; deduced optimal conditions for superheavy nuclei synthesis. Few cross sections compared to available data.

doi: 10.1140/epja/i2016-16305-9
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2015HO08 Phys.Rev. C 92, 014617 (2015)

J.Hong, G.G.Adamian, N.V.Antonenko

Influence of entrance channel on the production of hassium isotopes

NUCLEAR REACTIONS ²²⁶Ra(⁴⁸Ca, 3n), (⁴⁸Ca, 4n), (⁴⁸Ca, 5n), ²³²Th(⁴⁰Ar, 3n), (⁴⁰Ar, 4n), (⁴⁰Ar, 5n), ²³⁸U(³⁶S, 3n), (³⁶S, 4n), (³⁶S, 5n), (³⁴S, 3n), (³⁴S, 4n), (³⁴S, 5n), (²⁶Mg, 3n), (²⁶Mg, 4n), (²⁶Mg, 5n), ²⁴⁸Cm(²⁶Mg, 3n), (²⁶Mg, 4n), (²⁶Mg, 5n), (²⁵Mg, 3n), (²⁵Mg, 4n), (²⁵Mg, 5n), ²⁴⁴Pu(³⁰Si, 3n), (³⁰Si, 4n), (³⁰Si, 5n), ²⁴⁹Cf(²²Ne, 3n), (²²Ne, 4n), (²²Ne, 5n), E near and sub-barrier energies; calculated effective capture cross section and fusion probability P_CN, survival probabilities as function of the excitation energy of the compound nucleus, σ for 3n-, 4n- and 5n-channels leading to production of ^{266,267,268,269,270,271}Hs isotopes. Dinuclear system (DNS) model. Comparison with experimental data.

doi: 10.1103/PhysRevC.92.014617
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2014HO06 Phys.Rev. C 89, 034905 (2014)

J.Hong, P.H.Diamond

Anomalous viscosity of the quark-gluon plasma

doi: 10.1103/PhysRevC.89.034905
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2014HO13 Phys.Rev. C 90, 024605 (2014)

J.Hong, P.Danielewicz

Subthreshold pion production within a transport description of central Au + Au collisions

doi: 10.1103/PhysRevC.90.024605
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2012HO14 Phys.Rev. C 85, 064903 (2012)

J.Hong, D.Teaney, P.M.Chesler

Wake of a heavy quark in non-Abelian plasmas: Comparing kinetic theory and the anti-de Sitter space/conformal field theory correspondence

doi: 10.1103/PhysRevC.85.064903
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2011NU01 Phys.Rev. C 83, 034610 (2011)

F.M.Nunes, A.Deltuva, J.Hong

Improved description of ^{34, 36, 46}Ar( p, d) transfer reactions

NUCLEAR REACTIONS ¹H(³⁴Ar, d), (³⁶Ar, d), (⁴⁶Ar, d), E=33 MeV/nucleon; analyzed σ(θ), spectroscopic factors using finite range adiabatic wave approximation (ADWA) and Full three-body Faddeev calculations. Neutron-proton asymmetry dependence from knockout measurements.

doi: 10.1103/PhysRevC.83.034610
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2010HO14 Phys.Rev. C 82, 044908 (2010)

J.Hong, D.Teaney

Spectral densities for hot QCD plasmas in a leading-log approximation

doi: 10.1103/PhysRevC.82.044908
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