NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = A.A.Usmani Found 28 matches. 2023RA06 Eur.Phys.J.Plus 138, 467 (2023) A.A.Rather, M.Ikram, I.A.Rather, M.Imran, A.A.Usmani, B.Kumar, K.P.Santhosh, S.K.Patra Theoretical studies on structural properties and decay modes of 284-375119 isotopes RADIOACTIVITY 284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320,321,322,323,324,325,326,327,328,329,330,331,332,333,334,335,336,337,338,339,340,341,342,343,344,345,346,347,348,349,350,351,352,353,354,355,356,357,358,359,360,361,362,363,364,365,366,367,368,369,370,371,372,373,374,375119(α), (SF); calculated T1/2, binding energy, quadrupole deformation parameter, separation energies, density profile and shape co-existence within the axially deformed relativistic mean field with NL3* parametrisation.
doi: 10.1140/epjp/s13360-023-03959-6
2021RA09 Nucl.Phys. A1010, 122189 (2021) I.A.Rather, A.A.Usmani, S.K.Patra Effect of inner crust EoS on neutron star properties
doi: 10.1016/j.nuclphysa.2021.122189
2021RA11 Phys.Rev. C 103, 055814 (2021) I.A.Rather, U.Rahaman, M.Imran, H.C.Das, A.A.Usmani, S.K.Patra Rotating neutron stars with quark cores
doi: 10.1103/PhysRevC.103.055814
2020RA16 Int.J.Mod.Phys. E29, 2050044 (2020) I.A.Rather, A.Kumar, H.C.Das, M.Imran, A.A.Usmani, S.K.Patra Constraining bag constant for hybrid neutron stars
doi: 10.1142/S0218301320500445
2020RA18 J.Phys.(London) G47, 105104 (2020) I.A.Rather, A.A.Usmani, S.K.Patra Study of nuclear matter properties for hybrid EoS
doi: 10.1088/1361-6471/aba116
2020RA26 Int.J.Mod.Phys. E29, 2050076 (2020) U.Rahaman, M.Ikram, M.Imran, A.A.Usmani A study of nuclear radii and neutron skin thickness of neutron-rich nuclei near the neutron drip line NUCLEAR STRUCTURE Z=6-40; calculated two-neutron separation and binding energies, charge and root mean square neutron radii, nuclear asymmetry parameter, neutron skin-thickness.
doi: 10.1142/S0218301320500767
2018US01 Int.J.Mod.Phys. E27, 1850060 (2018) A.A.Usmani, S.A.Abbas, U.Rahaman, M.Ikram, F.H.Bhat The role of the elemental nature of A=3 nuclei in neutron-rich nuclei NUCLEAR STRUCTURE 24O, 60Ca, 105Br, 123Nb, 189Eu, 276U; calculated one- and two-triton separation energies, one- and two-neutron separation energies, binding energies; deduced six magic nuclei.
doi: 10.1142/S021830131850060X
2017AH03 Phys.Rev. C 95, 054601 (2017) S.Ahmad, A.A.Usmani, S.Ahmad, Z.A.Khan Interaction cross sections and matter radii of oxygen isotopes using the Glauber model NUCLEAR STRUCTURE 16,18,20,22,24,26O; calculated point proton and neutron density distributions, oscillator parameters, matter rms radii using Slater determinants consisting of the harmonic oscillator single-particle wave functions (SDHO) and relativistic mean-field approach (RMF). NUCLEAR REACTIONS 12C(16O, X), (18O, X), (20O, X), (22O, X), (24O, X), (26O, X), E=1.0 GeV/nucleon; calculated interaction σ. 16O(p, p), E=200, 300, 600, 1000 MeV; calculated σ(θ, E). 16O(p, X), E=40-1000 MeV; calculated reaction σ(E). Coulomb modified correlation expansion for Glauber model S matrix, and densities from the Slater determinants consisting of the harmonic oscillator single-particle wave functions (SDHO) and relativistic mean field (RMF) approach. Comparison with experimental data.
doi: 10.1103/PhysRevC.95.054601
2017AH08 Phys.Rev. C 96, 064602 (2017) Matter radii of light proton-rich and neutron-rich nuclear isotopes NUCLEAR REACTIONS 1H(α, α), E=650, 850 MeV; 1H(16O, 16O'), E=1000 MeV; analyzed experimental differential σ(θ) data. 12C(α, X), (6He, X), (8He, X), (7Li, X), (8Li, X), (9Li, X), (11Li, X), (9Be, X), (10Be, X), (11Be, X), (12Be, X), (14Be, X), (12B, X), (13B, X), (14B, X), (15B, X), E=790 MeV; 12C(10B, X), (13C, X), (16C, X), (19C, X), E=960 MeV; 12C(11B, X), (12C, X), (20Ne, X), (20O, X), (20F, X), (26F, X), (20Ne, X), (21Ne, X), (23Ne, X), (24Ne, X), (25Ne, X), (26Ne, X), (28Ne, X), (29Ne, X), (22Na, X), (23Na, X), (25Na, X), (26Na, X), (27Na, X), (28Na, X), (29Na, X), (30Na, X), (31Na, X), (32Na, X), (24Mg, X), (25Mg, X), (27Mg, X), (29Mg, X), (30Mg, X), (31Mg, X), (32Mg, X), E=950 MeV; 12C(17B, X), (19B, X), E=800 MeV; 12C(14C, X), (17C, X), (14N, X), (22N, X), (22O, X), (24F, X), E=965 MeV; 12C(15C, X), (17N, X), E=740 MeV; 12C(18C, X), E=955 MeV; 12C(20C, X), E=905 MeV; 12C(15N, X), (18F, X), E=975 MeV; 12C(16N, X), (18N, X), (23F, X), E=1020 MeV; 12C(19N, X), (21N, X), (24F, X), E=1005 MeV; 12C(23N, X), E=920 MeV; 12C(16O, X), (17O, X), (19O, X), E=970 MeV; 12C(18O, X), E=1050 MeV; 12C(21O, X), E=980 MeV; 12C(19F, X), E=985 MeV; 12C(21F, X), E=1000 MeV; 12C(25F, X), E=1010 MeV; calculated oscillator constants, proton and neutron rms radii, proton and neutron density distributions; predicted experimental cross sections of stable and neutron-rich nuclei on 12C. 4,6,8He, 6,7,8,9,11Li, 9,10,11,12,13,14Be, 10,11,12,13,14,15,16,17,19B, 12,13,14,15,16,17,18,19,20C, 14,15,16,17,18,19,20,21,22,23N, 16,17,18,19,20,21,22,23,24O, 18,19,20,21,23,24,25,26F, 20,21,23,24,25,26,28,29Ne, 22,23,25,27,28,29,30,31,32Na, 24,25,27,29,30,31,32Mg; extracted matter rms radii of neutron-rich nuclei, and compared with other theoretical approaches. 3He, 7Be, 8B, 9,10,11C, 12,13N, 13,14,15O, 17F, 17,18,19Ne, 19,20,21Na, 20,22,23Mg; extracted matter rms radii of proton-rich nuclei, and compared with other calculations. Glauber model.
doi: 10.1103/PhysRevC.96.064602
2016AH01 Eur.Phys.J. A 52, 128 (2016) S.Ahmad, D.Chauhan, A.A.Usmani, Z.A.Khan Study of the neon interaction cross section using the Glauber model NUCLEAR REACTIONS 12C(17Ne, x), (18Ne, x), (19Ne, x), (20Ne, x), (21Ne, x), (22Ne, x), (23Ne, x), (24Ne, x), (25Ne, x), (26Ne, x), (27Ne, x), (28Ne, x), (29Ne, x), (30Ne, x), (31Ne, x), (32Ne, x), E=240 MeV/nucleon; calculated Ne harmonic oscillator parameters, neutron and proton rms radii, interaction σ, 1n removal σ using Glauber model S-matrix. Compared to available data. 31Ne deduced neutron halo.
doi: 10.1140/epja/i2016-16128-8
2016RA40 Eur.Phys.J. A 52, 372 (2016) A.A.Rather, M.Ikram, A.A.Usmani, B.Kumar, S.K.Patra Structural and decay properties of Z = 132, 138 superheavy nuclei NUCLEAR STRUCTURE Z=132, 138; calculated binding energy, mass excess, deformation, radius vs neutron number, α-decay, β-decay, SF T1/2 using axially deformed relativistic mean-field with NL3*.
doi: 10.1140/epja/i2016-16372-x
2014CH39 Phys.Rev. C 90, 024603 (2014) D.Chauhan, Z.A.Khan, A.A.Usmani Interaction cross sections for neon isotopes in the Glauber model and the halo structure of 31Ne NUCLEAR REACTIONS 12C(17Ne, X), (18Ne, X), (19Ne, X), (20Ne, X), (21Ne, X), (22Ne, X), (23Ne, X), (24Ne, X), (25Ne, X), (26Ne, X), (27Ne, X), (28Ne, X), (29Ne, X), (30Ne, X), (31Ne, X), (32Ne, X), E=240, 950 MeV/nucleon; calculated interaction cross sections with and without the two-body density term. Halo structure. Coulomb-modified correlation expansion for the Glauber model S matrix. Comparison with experimental data. NUCLEAR STRUCTURE 17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32Ne; calculated point-proton and neutron RMF density distributions, neutron, proton, and matter radii.
doi: 10.1103/PhysRevC.90.024603
2014IM01 J.Phys.(London) G41, 065101 (2014) M.Imran, A.A.Usmani, M.Ikram, Z.Hasan, F.C.Khanna Fully correlated variational Monte Carlo study of 4ΛH and 4ΛH* hypernuclei NUCLEAR STRUCTURE 4H; calculated hypernuclei separation energy, quenching factors, energy splitting between 0+ and 1+ states, one-body density. Comparison with available data.
doi: 10.1088/0954-3899/41/6/065101
2008US01 J.Phys.(London) G35, 025105 (2008) Behaviour of the ΛN and ΛNN potential strengths in the 5ΛHe hypernucleus
doi: 10.1088/0954-3899/35/2/025105
2007US01 J.Phys.(London) G34, 2707 (2007) Behaviour of the potentials due to strangeness degree of freedom in 6Λ∓LHe hypernucleus
doi: 10.1088/0954-3899/34/12/014
2006US01 Phys.Rev. C 73, 011302 (2006) ΛN space-exchange correlation effects in the 5ΛHe hypernucleus NUCLEAR STRUCTURE 5He; calculated hypernucleus binding energy, radius, Λ-separation energy, related features; deduced sensitivity to space-exchange correlation.
doi: 10.1103/PhysRevC.73.011302
2006US03 Phys.Rev. C 74, 034320 (2006) Fully correlated study of 6ΛΛHe hypernucleus including ΛN space-exchange correlations NUCLEAR STRUCTURE 6He; calculated wave functions, core polarization, hyperon separation energies for two-Λ hypernuclei; deduced role of space-exchange correlations.
doi: 10.1103/PhysRevC.74.034320
2003US01 Phys.Rev. C 68, 024001 (2003) Variational Monte Carlo calculation of 5ΛHe hypernucleus NUCLEAR STRUCTURE 5He; calculated hypernucleus binding energy, one-body density, core polarization. Variational Monte Carlo technique.
doi: 10.1103/PhysRevC.68.024001
2000BE23 Nucl.Phys. A673, 241 (2000) O.Benhar, N.N.Nikolaev, J.Speth, A.A.Usmani, B.G.Zakharov Final State Interactions in 4He(e, e'p)3H at Large Proton Energy NUCLEAR REACTIONS 4He(e, e'p), E not given; calculated missing momentum distributions for large proton energy; deduced final state interaction effects, role of color transparency. Eikonal approximation.
doi: 10.1016/S0375-9474(00)00126-3
1996BE66 Z.Phys. A355, 267 (1996) O.Benhar, S.Fantoni, N.N.Nikolaev, J.Speth, A.A.Usmani, B.G.Zakharov Glauber Theory of Initial- and Final-State Interactions in (p, 2p) Scattering NUCLEAR REACTIONS 27Al(p, 2p), E at 6-12 GeV/c; 16O, 40Ca(p, 2p), E at 6, 12 GeV/c; calculated nuclear transparency vs missing momentum x-, y-compenents; analyzed data. Quasielastic scattering, initial, final states Glauber theory description.
doi: 10.1007/s002180050109
1996BF01 Zh.Eksp.Teor.Fiz. 110, 1933 (1996); J.Exper.Theo.Phys. 83, 1063 (1996) O.Benhar, S.Fantoni, N.N.Nikolaev, J.Speth, A.A.Usmani, B.G.Zakharov On the Missing-Momentum Dependence of the Color-Transparency Effects in (e, e'p) Scattering NUCLEAR REACTIONS 16O, 40Ca(e, e'p), E not given; calculated nuclear transparency, missing momentum distribution in parallel, transverse kinematics; deduced non-vanishing off diagonal incoherent rescattering contribution. Coupled-channel multiple-scattering theory.
1995BE50 Phys.Lett. 358B, 191 (1995) O.Benhar, S.Fantoni, N.N.Nikolaev, J.Speth, A.A.Usmani, B.G.Zakharov The Longitudinal Asymmetry of the (e, e'p) Missing Momentum Distribution as a Signal of Color Transparency NUCLEAR REACTIONS 16O, 40Ca(e, e'p), E not given; calculated longitudinal asymmetry vs Q2; deduced color transparency related features. Multiple scattering theory.
doi: 10.1016/0370-2693(95)01025-L
1995US01 Phys.Rev. C51, 2347 (1995) A.A.Usmani, S.C.Pieper, Q.N.Usmani Variational Calculations of the (Lambda)-Separation Energy of the 17O(Lambda) Hypernucleus NUCLEAR STRUCTURE A=17; calculated 17O(lambda) hypernucleus lambda separation energy. Variational Monte Carlo simulations.
doi: 10.1103/PhysRevC.51.2347
1995US02 Phys.Rev. C52, 1773 (1995) Three-Baryon ΛNN Potential NUCLEAR STRUCTURE 4He; calculated nucleons one-body densities. A=5; calculated nucleons one-body densities, for 5He(Λ) hypernucleus; deduced (Λ)(NN) potential strength. Three-baryon (Λ)(NN) potential, realistic variational Monte Carlo calculations.
doi: 10.1103/PhysRevC.52.1773
1992US01 Phys.Rev. C45, 396 (1992) A.A.Usmani, I.Ahmad, Q.N.Usmani 4He-4He Elastic Scattering and Variational Wave Functions NUCLEAR REACTIONS 4He(α, α), E at 4.32 GeV/c; analyzed data. Glauber multiple scattering theory, correlated variational wave functions.
doi: 10.1103/PhysRevC.45.396
1991US01 Phys.Rev. C43, 2412 (1991) Convergence of the Nucleus-Nucleus Glauber Multiple Scattering Series NUCLEAR REACTIONS 4He(α, α), E at 4.32 GeV/c; analyzed data; deduced model convergence features. Glauber S-matrix operator, multiple scattering series.
doi: 10.1103/PhysRevC.43.2412
1989US01 Phys.Rev. C39, 1182 (1989) A.A.Usmani, I.Ahmad, Q.N.Usmani α 4He Elastic Scattering at High Energies NUCLEAR REACTIONS 4He(α, α), E at 4.32, 5.07 GeV/c; calculated σ(θ) vs momentum. Glauber multiple scattering theory.
doi: 10.1103/PhysRevC.39.1182
1989US03 J.Phys.(London) G15, 1667 (1989) A Correction to the Rigid-Projectile Model NUCLEAR REACTIONS 12C, 40Ca(α, α), E=1.37 GeV; calculated σ(θ). Rigid projectile model.
doi: 10.1088/0954-3899/15/11/011
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