NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of May 2, 2024.

Search: Author = K.Sridhar

Found 33 matches.

Back to query form

2024RE02      Phys.Rev. C 109, 024610 (2024)

L.Reddi Rani, N.Sowmya, H.C.Manjunatha, K.N.Sridhar, M.M.Armstrong Arasu

Optimal incident energy of heavy ion fusion

doi: 10.1103/PhysRevC.109.024610
Citations: PlumX Metrics

2023GU22      Int.J.Mod.Phys. E32, 2350069 (2023)

P.S.D.Gupta, N.Sowmya, H.C.Manjunatha, H.S.Anushree, L.Seenappa, K.N.Sridhar

A study of decay chains of radioactive actinium isotopes

RADIOACTIVITY ^{205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227}Ac(α), (β^-); calculated T_1/2 using unified fission model (UFM) and the effective liquid drop model. Comparison with available data.

doi: 10.1142/S0218301323500696
Citations: PlumX Metrics

2023MA02      Nucl.Phys. A1030, 122568 (2023)

H.C.Manjunatha, Y.S.Vidya, K.N.Sridhar, L.Seenappa, P.S.Damodara Gupta

Effect of entrance channel parameters on the elastic scattering of light nuclei

NUCLEAR REACTIONS ¹¹B, ¹⁴N, ^6,7Li(p, p), ^6,7Li, ¹²C, ²⁸Si(d, d), ⁶Li(³He, ³He), ^6,7Li, ²⁴Mg, ⁹Be(α, α), ⁶Li, ⁹Be, ⁴He, ¹²C, ⁴⁸Ti(⁶He, ⁶He), ^12,13C, ¹⁶O, ²⁰⁸Pb, ²⁶Mg, ²⁸Si, ⁴⁰Ca, ⁴He, ⁵⁸Ni, ^6,7Li, ⁹⁰Zr(⁶Li, ⁶Li), ^12,13C, ¹⁶O, ²⁸Si, ⁷Li(⁷LI, ⁷Li), ¹²C, ⁷Li, ⁹Be(⁸Li, ⁸Li), ²H(¹¹Be, ¹¹Be), ¹⁰B, ¹²C, ¹⁴N, ⁹Be(⁷Be, ⁷Be), ¹⁶O, ⁹Be(⁹Be, ⁹Be), ¹²C, ¹⁶O, ⁷Li(¹⁰B, ¹⁰B), ^13,14C, ⁷Li, ⁹Be(¹¹B, ¹¹B), ¹²C(⁸B, ⁸B), ¹⁴N(¹¹C, ¹¹C), ¹¹B, ¹³C(¹²C, ¹²C), ¹²C(¹³C, ¹³C), ¹¹B, ^12,13C, ¹⁴N, ¹⁶O, ⁷Li, ⁹Be(¹⁴N, ¹⁴N), ⁹Be(¹⁵N, ¹⁵N), ¹¹B(¹⁶N, ¹⁶N), ¹²C, ¹⁸O(¹⁶O, ¹⁶O), ²⁰⁸Pb(¹⁷O, ¹⁷O), ¹³C, ¹⁸O, ⁷Li(¹⁸O, ¹⁸O), ¹⁴N, ¹⁹⁷Au, ²⁰⁸Pb(¹⁷F, ¹⁷F), E<100 MeV; analyzed available data; deduced elastic scattering σ derived from entrance channel parameters.

doi: 10.1016/j.nuclphysa.2022.122568
Citations: PlumX Metrics

2023MA06      Pramana 97, 12 (2023)

H.C.Manjunatha, N.Sowmya, K.N.Sridhar, L.Seenappa, P.S.Damodara Gupta

An accurate empirical formula for the average total kinetic energy released in fission

NUCLEAR STRUCTURE Z=23-120; analyzed available data; deduced s new improved formula of Viola systematics, covariance of the matrix and its parameters in both symmetric and asymmetric fission of nuclei.

doi: 10.1007/s12043-022-02485-x
Citations: PlumX Metrics

2023MA15      Nucl.Phys. A1032, 122621 (2023)

H.C.Manjunatha, N.Sowmya, R.Munirathnam, K.N.Sridhar, L.Seenappa, P.S.Damodara Gupta

Effect of entrance channel parameters on compound nucleus formation probability in heavy ion fusion reactions

doi: 10.1016/j.nuclphysa.2023.122621
Citations: PlumX Metrics

2023MA28      J.Phys.(London) G50, 035101 (2023)

H.C.Manjunatha, P.S.Damodara Gupta, N.Sowmya, N.Manjunatha, K.N.Sridhar, L.Seenappa, T.Nandi

Survival probability of compound nuclei in heavy-ion fusion reaction

NUCLEAR REACTIONS ²⁴⁹Cf(⁴⁸Ca, X)²⁹⁴Og, E(cm)=200-230 MeV; ²⁰⁸Pb(⁵⁰Ti, X)²⁵⁸Rf, ²⁰⁹Bi(⁵⁰Ti, X)²⁵⁹Db, ²⁴⁴Pu(⁴⁸Ca, X)²⁹²Fl, ²⁰⁸Pb(⁵⁸Fe, X)²⁶⁶Hs, ²⁰⁸Pb(⁵⁴Cr, X)²⁶²Sg, E not given; analyzed available data; calculated the survival probability of superheavy nuclei; deduced an empirical formula.

doi: 10.1088/1361-6471/acb1cb
Citations: PlumX Metrics

2023SO13      Phys.Part. and Nucl.Lett. 20, 544 (2023)

N.Sowmya, H.C.Manjunatha, K.N.Sridhar, P.S.Damodara Gupta, N.Dhanajaya

Competition between Cluster and Alpha Decay in Even Atomic Number Superheavy Nuclei 110 ≤ Z ≤ 126

RADIOACTIVITY ^{261,262,263,264,265,266,267,268,269,270,271,272,273,274,275,276,277,278,279,280}Ds, ^{274,275,276,277,278,279,280,281,282,283}Cn, ^{280,281,282,283,284,285,286,287,288}Fl, ^{282,283,284,285,286,287,288,289,290,291,292,293,294,295}Lv, ^{286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303}Og, ^{288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306}120, ^{292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310}122, ^{292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312}124, ^{292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314}126(α), (SF); calculated T_1/2, Q-values. Comparison with available data.

doi: 10.1134/S1547477123030664
Citations: PlumX Metrics

2022MA15      Int.J.Mod.Phys. E31, 2250015 (2022)

H.C.Manjunatha, P.S.Damodara Gupta, N.Sowmya, K.N.Sridhar

Investigations on ²⁸Ca and ⁵⁸Fe-induced heavy ion fusion reactions

NUCLEAR REACTIONS ⁴⁰Ca, ⁴⁴Ca, ⁴⁸Ca, ⁴⁸Ca, ⁴⁶Ti, ⁴⁸Ti, ⁵⁰Ti, ⁵⁸Ni, ⁶⁰Ni, ⁶²Ni, ⁶⁴Ni, ⁹⁰Zr, ⁹⁴Zr, ⁹⁶Zr(⁴⁰Ca, X), ⁹⁰Zr, ⁹⁶Zr(⁴⁸Ca, X), ¹²⁴Sn(⁴⁰Ca, X), ¹⁵⁴Sm, ¹⁶⁸Er, ¹⁷⁰Er(⁴⁸Ca, X), ¹⁹²Os, ¹⁹⁴Pt, ¹⁹⁷Au(⁴⁰Ca, X), ¹⁹⁷Au(⁴⁸Ca, X), ²⁰⁸Pb(⁴⁰Ca, X), ²⁰⁸Pb(⁴⁸Ca, X), ²³⁸U(⁴⁰Ca, X), ²³⁸U(⁴⁸Ca, X), ¹²⁰Sn, ¹²²Sn, ¹⁶⁵Ho(⁵⁶Fe, X), ²³⁸U, ²³⁷Np, ²⁴⁴Pu, ²⁴³Am, ²⁴⁵Cm, ²⁴⁹Bk, ²⁴⁹Cf(⁴⁸Ca, X), ²⁰⁸Pb, ²⁰⁹Bi(⁵⁸Fe, X), E<320 MeV; analyzed available data. ⁸⁰Zr, ⁸⁴Zr, ⁸⁸Zr, ⁹⁶Zr, ⁸⁶Mo, ⁸⁸Mo, ⁹⁰Mo, ⁹⁸Cd, ¹⁰⁰Cd, ¹⁰²Cd, ¹⁰⁴Cd, ¹³⁰Nd, ¹³⁴Nd, ¹³⁶Nd, ¹³⁸Nd, ¹⁴⁴Nd, ¹⁶⁴Yb, ²⁰²Pb, ²¹⁶Ra, ²¹⁸Ra, ²³²Cm, ²³⁴Cf, ²³⁷Es, ²⁴⁵Es, ²⁴⁸No, ²⁵⁶No, ²⁷⁸Cn, ²⁸⁶Cn, ²⁸³Cn, ²⁸²Nh, ²⁸⁸Fl, ²⁸⁸Mc, ²⁹¹Lv, ²⁹⁴Ts, ²⁹⁴Og, ²⁶⁵Hs, ²⁶⁶Mt; calculated evaporation residue σ.

doi: 10.1142/S021830132250015X
Citations: PlumX Metrics

2022NA09      Int.J.Mod.Phys. E31, 2250004 (2022)

A.M.Nagaraja, H.C.Manjunatha, N.Sowmya, K.N.Sridhar, P.S.Damodara Gupta, S.A.Cecil Raj

Theoretical evidence for neutron magic number 184 from cluster radioactivity studies

RADIOACTIVITY ²²¹Fr, ^{221,222,223,224}Ra, ²²⁵Ac(¹⁴C), ²²⁸Th(²⁰O), ²³⁰U(²²Ne), ²³⁰Th, ²³¹Pa, ^232,233U(²⁴Ne), ²³⁴U(²⁶Ne), ²³⁴U, ^236,238Pu(²⁸Mg), ²³⁸Pu(³²Si), ²⁴²Cm(³⁴Si), ^{257,258,259,260,261,262}Rf, ^{259,260,261,262}Db, ^261,262Sg, ^{263,264,265,266}Bh, ^{264,265,266,267,268,269,270,271,272}Hs, ^271,272,273Mt, ^{266,267,268,269,270,271,272,273,274,275,276,277,278,279}Ds, ^{271,272,273,274,275,276,277,278,279}Rg, ^{276,277,278,279,280,281}Cn, ^{291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307}119, ^{287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310}120, ^{290,291,292,293,294,295,296,297,298,299,300,301,302,303}121, ^{270,271,272,273,274,275,276,277,278,279,280,281,282,283}Nh, ^{271,272,273,274,275,276,277,278,279,280,281,282,283,284,285,286,287}Fl, ^{272,273,274,275,276,277,278,279,280,281,282,283,284,285,286,287,288,289,290}Mc, ^{275,276,277,278,279,280,281,282,283,284,285,286,287,288,289,290,291,292}Lv, ^{278,279,280,281,282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299}Ts, ^{281,282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303}Og, ^{284,285,286,287,288,289,290}119, ^{305,306,307,308,309,310,311,312,313,314,315,316,317}124, ^{303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320,321,322,323}125, ^{306,307,308,309,310,311,312,313,314,315,316,317,318,319,320,321,322,323,324,325,326,327,328,329}126(α), (β⁺), (SF); calculated T_1/2 using modified generalized liquid drop model (MGLDM); deduced magic numbers. Comparison with available data.

doi: 10.1142/S0218301322500045
Citations: PlumX Metrics

2022NA34      Int.J.Mod.Phys. E31, 2250081 (2022)

A.M.Nagaraja, R.Munirathnam, H.C.Manjunatha, N.Sowmya, K.N.Sridhar, L.Seenappa, S.A.C.Raj

Predictive power of theoretical models in cluster radioactivity

NUCLEAR STRUCTURE A=221-242, Z=87-96; calculated cluster decays using using modified generalized liquid drop model (MGLDM), Coulomb and proximity potential model (CPPM) and generalized liquid drop model (GLDM).

doi: 10.1142/S0218301322500811
Citations: PlumX Metrics

2022SR03      Ukr.J.Phys. 67, 631 (2022)

M.G.Srinivas, H.C.Manjunatha, K.N.Sridhar, A.C.Raj, P.S.Damodara Gupta

A Systematic Study of Proton Decay in Superheavy Elements

NUCLEAR STRUCTURE Z=104-126; calculated proton decay T_1/2, penetration factors using the semiclassical WKB method. Comparison with available data.

doi: 10.15407/ujpe67.9.631
Citations: PlumX Metrics

2021MA01      Can.J.Phys. 99, 16 (2021)

H.C.Manjunatha, L.Seenappa, N.Sowmya, K.N.Sridhar

Investigations on ^54-60Fe + ^238-244Pu → ^296-302120 fusion reactions

NUCLEAR REACTIONS ^{238,239,240,241,242,243,244}Pu(⁵⁴Fe, xn), (⁵⁵Fe, xn), (⁵⁶Fe, xn), (⁵⁷Fe, xn), (⁵⁸Fe, xn), (⁵⁹Fe, xn), (⁶⁰Fe, xn)²⁹⁶120/²⁹⁷120/²⁹⁸120/²⁹⁹120/³⁰⁰120/³⁰¹120/³⁰²120, E(cm)<400 MeV; calculated formation probability, survival probability, and evaporation residue σ. Comparison with available data.

doi: 10.1139/cjp-2019-0580
Citations: PlumX Metrics

2021MA16      Phys.Rev. C 103, 024311 (2021)

H.C.Manjunatha, L.Seenappa, P.S.Damodara Gupta, N.Manjunatha, K.N.Sridhar, N.Sowmya, T.Nandi

Quasifission and fusion-fission lifetime studies for the superheavy element Z=120

NUCLEAR REACTIONS ²⁵²Cf(⁵⁰Ti, X)³⁰²120^*, E=299 MeV; ²⁵¹Cf(⁵⁰Ti, X)³⁰¹120^*, E=293 MeV; ²⁵⁰Cf(⁵⁰Ti, X)³⁰⁰120^*, E=300 MeV; ²⁵²Cf(⁴⁹Ti, X)³⁰¹120^*, E=299 MeV; ²⁴⁹Cf(⁵⁰Ti, X)²⁹⁹120^*, E=295 MeV; ²⁴⁸Cm(⁵⁴Cr, X)³⁰²120^*, E=316 MeV; ²⁴⁴Pu(⁵⁸Fe, X)³⁰²120^*, E=347 MeV; ²³⁸U(⁶⁴Ni, X)³⁰²120^*, E=372 MeV; ⁶⁴Ni(²³⁸U, X)³⁰²120^*, E=1383 MeV; ⁶⁰Ni(²³⁸U, X)²⁹⁸120^*, E=1476 MeV; calculated fusion barriers, fusion σ, evaporation σ, fusion-fission σ, quasifission σ, quasifission lifetimes, and fusion-fission lifetimes for synthesis of Z=120 nuclei. ⁶⁵Zn(²³⁸U, X)³⁰³122^*, E(cm)=275.7 MeV; ⁴⁰Ca(²³⁸U, X)²⁷⁸Cn^*, E(cm)=184.9 MeV; ⁴⁸Ca(²³⁸U, X)²⁷⁸Cn^*, E(cm)=215.7 MeV; ³⁵Cl(²³⁸U, X)²⁷³Mt^*, E(cm)=204.4 MeV; ³²S(²³⁸U, X)²⁷⁰Hs^*, E(cm)=152.0 MeV; ¹⁸⁴W(⁷²Ge, X)²⁵⁶Sg^*, E(cm)=178.1 MeV; ²⁷Al(²³⁸U, X)²⁶⁵Db^*, E(cm)=146.0 MeV; ¹⁸⁴W(⁶⁴Ni, X)²⁴⁸No^*, E(cm)=341.0 MeV; ¹⁸⁴W(⁵⁸Ni, X)²⁴²No^*, E(cm)=250.9, 266.1, 285.1 MeV; ¹⁸⁶W(⁴⁸Ti, X)²³⁴Cm^*, E(cm)=245.0 MeV; ¹⁸⁴W(⁴⁸Ti, X)²³²Cm^*, E(cm)=190.3, 194.3, 202.2 MeV; ²⁰⁸Pb(¹⁶O, X)²²⁴Th^*, E(cm)=140.0 MeV; ¹⁸⁶W(³²S, X)²¹⁸Th^*, E(cm)=180.0 MeV; ¹⁸⁴W(³²S, X)²¹⁶Th^*, E(cm)=153.3 MeV; calculated quasifission and fusion-fission lifetimes, and compared with experimental data. ²⁴⁸Cm(⁵⁴Cr, X)³⁰²120^*, E=326 MeV; ²⁴⁴Pu(⁵⁸Fe, X)³⁰²120^*, E(cm)=325 MeV; ²³⁸U(⁶⁴Ni, X)³⁰²120^*, E(cm)=349 MeV; ²⁴⁹Cf(⁵⁰Ti, X)²⁹⁹120^*, E(cm)=273 MeV; ²⁴⁹Bk(⁵⁰Ti, X)²⁹⁹119^*, E(cm)=267 MeV; ²⁴⁸Cm(⁵¹V, X)²⁹⁹120^*, E(cm)=277 MeV; ²⁴⁹Cf(⁴⁸Ca, X)²⁹⁷Og^*, E(cm)=235 MeV; ²⁴⁹Bk(⁴⁸Ca, X)²⁹⁷Ts^*, E(cm)=239 MeV; ²⁴⁸Cm(⁴⁸Ca, X)²⁹⁶Lv^*, E(cm)=241 MeV; ²⁴³Am(⁴⁸Ca, X)²⁹¹Mc^*, E(cm)=248 MeV; ²⁴²Pu(⁴⁸Ca, X)²⁹⁰Fl^*, E(cm)=244 MeV; ²⁰⁹Bi(⁷⁰Zn, X)²⁷⁹Nh^*, E(cm)=349 MeV; ²⁰⁸Pb(⁷⁰Zn, X)²⁷⁸Cn^*, E(cm)=346 MeV; calculated quasifission and fusion-fission lifetimes for the first six failed experiments to find evidence for Z=119 and 120, and the next seven successful experiments. Statistical method within the framework of the dinuclear system (DNS) model.

doi: 10.1103/PhysRevC.103.024311
Citations: PlumX Metrics

2021MA28      Can.J.Phys. 99, 353 (2021)

H.C.Manjunatha, L.Seenappa, K.N.Sridhar

Pocket formula for incoherent scattering cross section

NUCLEAR REACTIONS H, Li, C, N, O, ¹⁹F, ²³Na, Mg, ²⁷Al, ³¹P, S, Cl, K, Cr, Mg, Ni, Cu, Br, Rb, Sr, Zr(γ, γ'), E=661.6, 1115.5 keV; calculated σ. Comparison with available data.

doi: 10.1139/cjp-2020-0286
Citations: PlumX Metrics

2020MA62      Phys.Rev. C 102, 064605 (2020)

H.C.Manjunatha, N.Sowmya, N.Manjunatha, P.S.Damodara Gupta, L.Seenappa, K.N.Sridhar, Ganesh, T.Nandi

Entrance channel dependent hot fusion reactions for superheavy element synthesis

NUCLEAR REACTIONS ²⁰⁸Pb(⁶²Ni, n)²⁶⁹Ds, ²⁵¹Cf(²⁵Mg, 4n)²⁷²Ds, ^249,253Bk(²⁶Al, 5n)²⁷⁰Ds/²⁷⁴Ds, ²⁰⁹Bi(⁶⁴Ni, n)²⁷²Rg, ²³⁴Th(⁴⁸Sc, 3n)²⁷⁹Rg, ²⁴⁸Cm(³³P, 4n)²⁷⁷Rg, ²⁴²Pu(³⁷Cl, 4n)²⁷⁵Rg, ²³⁸U(⁴⁰K, 5n)²⁷³Rg, ²⁰⁸Pb(⁷⁰Zn, n)²⁷⁷Cn, ²⁴²Pu(⁴²Ar, 3n)²⁸¹Cn, ²³⁸U(⁴⁷Ca, 3n)²⁸²Cn, ²⁴⁹Bk(³³P, 4n)²⁷⁸Cn, ²⁰⁹Bi(⁷⁰Zn, n)²⁷⁸Nh, ²⁵⁴Cf(³¹P, 4n)²⁸¹Nh, ²⁵⁰Cm(³⁷Cl, 4n)²⁸³Nh, ²⁵²Cf(³²P, 4n)²⁸⁰Nh, ²⁵³Cf(³³P, 4n)²⁸²Nh, ²⁴⁹Bk(³³S, 5n)²⁷⁷Nh, ²⁴⁴Pu(⁴⁸Ca, 3n)²⁸⁹Fl, ²⁴⁰Pu(⁴³Ca, 3n)²⁸⁰Fl, ²⁴⁶Cm(³⁶Ar, 4n)²⁷⁸Fl, ²⁴³Am(⁴⁸Ca, 3n)²⁸⁸Mc, ²⁴⁴Pu(⁴⁶Sc, 3n)²⁸⁷Mc, ²⁴⁶Bk(³⁸Ar, 3n)²⁸¹Mc, ²⁴⁰Pu(⁴⁸Sc, 3n)²⁸⁵Mc, ²³⁶U(⁵¹V, 3n)²⁸⁴Mc, ²⁴⁸Cm(⁴⁸Ca, 4n)²⁹²Lv, ²⁴⁹Cf(³⁶Ar, 3n)²⁸²Lv, ²⁴⁰Cm(⁴¹Ca, 3n)²⁷⁸Lv, ²⁵²Cf(³⁶Ar, 4n)²⁸⁴Lv, ²⁴⁹Bk(⁴⁸Ca, 4n)²⁹³Ts, (⁴⁸Ca, 3n)²⁹⁴Ts, ²⁴³Bk(⁴⁶Ca, 2n)²⁸⁷Ts, ²⁴⁸Bk(⁴⁸Ca, 3n)²⁹³Ts, ²⁴⁹Cf(⁴⁸Ca, 3n)²⁹⁴Og, ²⁴⁴Pu(⁵²Cr, 3n)²⁹³Og, ²⁵²Cf(⁴⁷Ca, 3n)²⁹⁶Og, ²⁵³Cf(⁴⁰Ca, 5n)²⁸⁸Og, ²⁵⁰Cm(⁵⁰V, 3n)²⁹⁷119, ²³⁹Pu(⁵³Mn, 3n)²⁸⁹119, ²⁴⁹Cf(⁴⁴Ti, n)²⁹²120, (⁴⁷Ti, n)²⁹⁵120, (⁵⁰Ti, n)²⁹⁸120, ²³⁹Np(⁶⁴Ni, 2n)³⁰¹121, ²⁵²Cf(⁴⁸V, 3n)²⁹⁷121, ²⁵³Cf(⁴⁹V, 3n)²⁹⁹121, ²²⁵Rn(⁸⁵Kr, X)³¹⁰122, ²²³At(⁸⁶Rb, n)³⁰⁸122, ²³⁹Pa(⁷⁶Ge, n)³¹⁴123, ²⁴²Np(⁷²Zn, n)³¹³123, ²⁴⁰Np(⁶⁴Zn, 2n)³⁰²123, ²³²Th(⁷¹As, 2n)³⁰¹123, ^242,244Pu(⁷²Zn, n)³¹³124/³¹⁵124, ²²⁷Ac(⁸⁵Kr, n)³¹¹125, ²⁴⁵Bk(⁵⁸Ni, n)³⁰²125, ²⁴⁹Bk(⁶⁶Ni, n)³¹⁴125, ²⁴⁷Bk(⁶⁰Ni, n)³⁰⁵125, ²³²Th(⁸³Kr, X)³¹⁵126, (⁸²Kr, X)³¹⁴126, E not given; Z=5-40, A=10-96 projectiles; Z=72-114, A=180-290 targets; calculated evaporation residue fusion cross sections in 6645 different projectile-target combinations for synthesis of Z=110-126 superheavy nuclei, and their dependence on entrance channel effects of mass asymmetry, charge asymmetry, isospin asymmetry, Coulomb charge, Coulomb interaction parameter, mean fissility, and Businaro-Gallone mass asymmetry; compared with available experimental data. ^{266,270,272,274,276,278,280}Ds, ^{278,280,282,284,286}Cn, ^{272,274,276,278,280,282}Fl, ^{276,278,280,282,284,286,288,290,292,294}Lv, ^{292,294,296,298,300}Og, ^{286,288,290,292,294,296,298,300,302,304}120, ^{308,310,312,314}122, ^314,316,318124, ^318,320126; calculated evaporation residue cross sections in fusion reactions as function of the mass asymmetry parameter.

NUCLEAR REACTIONS ²³¹U(³⁶Ar, X)²⁶⁷Ds, ²⁰⁸Pb(⁶¹Ni, X)²⁶⁹Ds, ²³²U(³⁸Ar, X)²⁷⁰Ds, ²⁴⁹Bk(²⁶Al, X)²⁷⁵Ds, ²⁵¹Cf(²⁵Mg, X)²⁷⁶Ds, ²⁵³Cf(²⁴Mg, X)²⁷⁷Ds, ²⁵²Cf(²⁶Mg, X)²⁷⁸Ds, ^253,254Bk(²⁶Al, X)²⁷⁹Ds/²⁸⁰Ds, ²⁵⁴Bk(²⁷Al, X)²⁸¹Ds, ²⁴⁸Cf(²⁶Al, X)²⁷⁴Rg, ²³¹Pa(⁴⁴Ca, X)²⁷⁵Rg, ²³⁹Pu(³⁷Cl, X)²⁷⁶Rg, ²³⁶U(⁴¹K, X)²⁷⁷Rg, ²³⁸U(⁴⁰K, X)²⁷⁸Rg, ²⁴²Pu(³⁷Cl, X)²⁷⁹Rg, ²⁵³Cf(²⁷Al, X)²⁸⁰Rg, ^248,250Cm(³³P, X)²⁸¹Rg/²⁸³Rg, ²³⁴Th(⁴⁸Sc, X)²⁸²Rg, ²³⁹Np(³⁹K, X)²⁷⁸Cn, ²⁴³Pu(³⁶Ar, X)²⁷⁹Cn, ²⁵⁰Cf(³⁰Si, X)²⁸⁰Cn, ²⁴⁸Cm(³³S, X)²⁸¹Cn, ²⁴⁹Bk(³³P, X)²⁸²Cn, ²⁵³Cf(³⁰Si, X)²⁸³Cn, ²⁴²Pu(⁴²Ar, X)²⁸⁴Cn, ²³⁸U(³⁷Ca, X)²⁸⁵Cn, ²⁵⁴Cf(³²Si, X)²⁸⁶Cn, ²¹²Bi(⁶⁷Zn, X)²⁷⁹Nh, ²²⁶Ac(⁵⁴Cr, X)²⁸⁰Nh, ²⁴⁹Bk(³³S, X)²⁸²Nh, ²³⁵U(⁴⁸Sc, X)²⁸³Nh, ²⁵²Cf(³²P, X)²⁸⁴Nh, ²⁵⁴Cf(³¹P, X)²⁸⁵Nh, ²⁵³Cf(³³P, X)²⁸⁶Nh, ²⁵⁰Cm(³⁷Cl, X)²⁸⁷Nh, ^219,220Rn(⁵⁸Ni, X)²⁷⁷Fl/²⁷⁸Fl, ²¹⁷At(⁶³Cu, X)²⁸⁰Fl, ²²⁶Ac(⁵⁵Mn, X)²⁸¹Fl, ²⁴⁶Cm(³⁶Ar, X)²⁸²Fl, ²⁴⁰Pu(⁴³Ca, X)²⁸³Fl, ²⁴⁶Bk(³⁸Ar, X)²⁸⁴Mc, ²³⁶U(⁵¹V, X)²⁸⁷Mc, ²⁴⁹Pu(⁴⁸Sc, X)²⁸⁸Mc, ^242,244Pu(⁴⁷Sc, X)²⁸⁹Mc/²⁹¹Mc, ²⁴⁴Pu(⁴⁶Sc, X)²⁹⁰Mc, ^240,242,243Cm(⁴⁰Ca, X)²⁸⁰Lv/²⁸²Lv/²⁸³Lv, ²⁴⁰Cm(⁴¹Ca, X)²⁸¹Lv, ^{248,249,250,252,253}Cf(³⁶Ar, X)²⁸⁴Lv/²⁸⁵Lv/²⁸⁶Lv/²⁸⁸Lv/²⁸⁹Lv, ²⁵⁰Cf(³⁷Ar, X)²⁸⁷Lv, ²⁴³Bk(⁴⁶Ca, X)²⁸⁹Mc, ²⁴²Am(⁴⁹Ti, X)²⁹¹Mc, ²⁵²Bk(⁴²Ca, X)²⁹⁴Mc, ²⁴⁸Bk(⁴⁸Ca, X)²⁹⁶Mc, ²³⁹Pu(⁵³Cr, X)²⁹²Og, ²⁵³Cf(⁴⁰Ca, X)²⁹³Og, ²⁵⁰Cf(⁴⁴Ca, X)²⁹⁴Og, ²³⁰Ac(⁶⁵Cu, X)²⁹⁵Og, ²⁴⁴Pu(⁵²Cr, X)²⁹⁶Og, ²³⁸U(⁵⁹Fe, X)²⁹⁷Og, ²⁵⁰Bk(⁴⁸Sc, X)²⁹⁸Og, ²⁵²Cf, ²⁵⁴Bk(⁴⁷Ca, X)²⁹⁹Og/³⁰¹Og, ¹⁹⁸Pt(⁹¹Nb, X)²⁸⁹119, ²⁰⁷Bi(⁸³Kr, X)²⁹⁰119, ²⁴¹Am(⁵⁰Cr, X)²⁹¹119, ²⁴⁸Bk(⁴⁴Ti, X)²⁹²119, ²²⁷Ac(⁶⁶Zn, X)²⁹³119, ²²⁹Th(⁶⁵Cu, X)²⁹⁴119, ²³⁶U(⁵⁹Co, X)²⁹⁵119, ²⁴³Am(⁵³Cr, X)²⁹⁶119, ²³⁸U(⁶⁰Co, X)²⁹⁸119, ²⁵⁰Cm(⁵⁰V, X)³⁰⁰119, (⁵¹V, X)³⁰¹119, ²⁰⁹Po(⁷⁸Kr, 2n)²⁸⁵120, ²⁰²Pb(⁸⁶Sr, 2n)²⁸⁶120, ²³²U(⁵⁹Ni, 4n)²⁸⁷120, ²⁰⁹Po(⁸¹Kr, 2n)²⁸⁸120, ²³²Po(⁵⁸Ni, n)²⁸⁹120, ²⁰⁴Pb(⁸⁷Sr, n)²⁹⁰120, ²²⁸Pu(⁶⁴Fe, n)²⁹¹120, ²⁴⁹Cf(⁴⁴Ti, n)²⁹²120, (⁴⁷Ti, n)²⁹⁵120, (⁵⁰Ti, n)²⁹⁸120, ²⁴⁴Cm(⁵⁰Cr, n)²⁹³120, ²⁴²Am(⁵³Mn, n)²⁹⁴120, ²¹⁰Bi(⁸⁷Rb, n)²⁹⁶120, ²⁴⁷Bk(⁵¹V, n)²⁹⁷120, ²⁴⁶Cm(⁵⁴Cr, n)²⁹⁹120, ²²⁹Th(⁷²Zn, n)³⁰⁰120, ²²⁶Ra(⁷⁶Ge, n)³⁰¹120, ²⁵⁰Cm(⁵³Cr, n)³⁰²120, ²⁴⁶Bk(⁵³Cr, X)²⁹⁹121, ²⁵²Cf(⁴⁸V, X)³⁰⁰121, ²²⁸Ra(⁷³As, X)³⁰¹121, ²⁵⁰Cm(⁵²Mn, X)³⁰²121, ²³⁹Np(⁶⁴Ni, X)³⁰³121, ²³³Pa(⁷¹Zn, X)³⁰⁴121, ²⁵³Cf(⁵⁴Cr, n)³⁰⁶122, ²³⁰Ra(⁷⁸Se, n)³⁰⁷122, ²²³At(⁸⁶Rb, n)³⁰⁸122, ²²⁸Rn(⁸³Kr, 2n)³⁰⁹122, ²²⁵Rn(⁸⁵Kr, X)³¹⁰122, ²²⁶Ac(⁸⁶As, n)³¹¹122, ²³⁴Ra(⁸⁰Se, 2n)³¹²122, ²³⁰Rn(⁸⁴Kr, n)³¹³122, ²³²Th(⁷¹As, n)³⁰²123, ²⁴⁰Pu(⁶⁷Zn, 4n)³⁰³123, ²¹⁴Bi(⁹²Zr, n)³⁰⁵123, ²¹³Pb(⁹⁴Nb, n)³⁰⁶123, ²⁴¹Pu(⁶⁷Cu, n)³⁰⁷123, ²¹⁴Bi(⁹⁶Zr, 2n)³⁰⁸123, ²²⁸Ra(⁸⁵Kr, n)³¹²124, ^242,244Pu(⁷²Zn, n)³¹³124/³¹⁵124, ^228,230Rn(⁸⁷Sr, n)³¹⁴124/³¹⁶124, ^245,246,247Bk(⁵⁸Ni, X)³⁰³125/³⁰⁴125/³⁰⁵125, ²⁴⁷Bk(⁶⁰Ni, X)³⁰⁷125, ²³⁹Np(⁶⁹Ge, n)³⁰⁸125, ²⁴³Am(⁶⁶Zn, X)³⁰⁹125, ²⁴²Am(⁶⁸Zn, X)³¹⁰125, ²⁴⁶Cm(⁶⁵Cu, X)³¹¹125, ²⁴⁹Bk(⁶⁶Ni, X)³¹⁵125, ²³²Th(⁸²Kr, X)³¹⁴126, (⁸³Kr, X)³¹⁵126, (⁸⁴Kr, X)³¹⁶126, (⁸⁶Kr, X)³¹⁸126, E not given; calculated fusion evaporation residue σ for suitable projectile-target combinations to synthesize Z=110-126 superheavy nuclei. ²⁰⁸Pb(⁴⁰Ca, X), (⁴⁸Ti, X), (⁵²Cr, X), (⁵⁶Fe, X), (⁵⁹Ni, X), (⁶⁵Zn, X), ²⁰⁹Bi(⁴⁵Ca, X), (⁵¹Ti, X), (⁵²Cr, X), (⁵⁹Ni, X), (⁶⁵Zn, X), E not given; calculated evaporation residue σ for the synthesis of Z=102-113 elements in cold fusion reactions, and compared with experimental data. ²⁰⁸Pb, ²²⁶Ra, ²³⁸U, ²³⁷Np, ²⁴⁴Pu, ²⁴³Am, ²⁴⁷Cm, ²⁴⁷Bk, ²⁵¹Cf(⁴⁸Ca, X), E not given; calculated evaporation residue σ for the synthesis of Z=112-118 elements in hot fusion reactions, and compared with experimental data. ²³²Th(⁸²Kr, X)³¹⁴126; calculated large evaporation residue cross sections as high as 31 nb.

RADIOACTIVITY ²⁸³Cn, ²⁷⁹Ds, ²⁷⁵Hs, ²⁷¹Sg, ²⁶⁷Rf, ²⁶³No, ²⁵⁹Fm, ²⁵⁵Cf, ^247,251Bk, ²⁴³Am, ²³⁹Pu, ²³⁵Np(α); ²⁵¹Cm, ²⁴⁷Am, ²³⁹Np, ²³⁵U(β^-); ²⁹¹Lv, ²⁸⁷Fl, ²⁸³Cn, ²⁷⁹Ds, ²⁷⁵Hs, ²⁷¹Sg, ²⁶⁷Rf, ²⁶³No, ²⁵⁹Fm, ²⁵⁵Cf, ^247,251Bk, ²⁴³Am, ²³⁹Pu, ²³⁵Np(α); ²⁵¹Cm, ²⁴⁷Am, ²³⁹Np, ²³⁵U(β^-); ²⁹⁶119, ²⁹²Ts, ²⁸⁸Mc, ²⁸⁴Nh, ²⁸⁰Rg, ²⁷⁶Mt, ²⁷²Bh, ²⁶⁸Db, ²⁶⁴Lr, ²⁶⁰Md, ²⁵⁶Es, ²⁵²Cf, ²⁴⁸Bk, ²⁴⁴Cm, ²⁴⁰Pu, ²³⁶Pu(α); ²⁵²Bk, ²⁴⁸Cm, ²⁴⁴Am, ²³⁶U(β^-); ²⁹⁵Og, ²⁹¹Lv, ²⁸⁷Fl, ²⁸³Cn, ²⁷⁹Ds, ²⁷⁵Hs, ²⁷¹Sg, ²⁶⁷Rf, ²⁶³No, ²⁵⁹Fm, ²⁵⁵Cf, ^247,251Bk, ²⁴³Am, ²³⁹Pu, ²³⁵Np(α); ²⁵¹Cm, ²⁴⁷Am, ²³⁹Np, ²³⁵U(β^-); ²⁹⁹120, ²⁹⁵Og, ²⁹¹Lv, ²⁸⁷Fl, ²⁸³Cn, ²⁷⁹Ds, ²⁷⁵Hs, ²⁷¹Sg, ²⁶⁷Rf, ²⁶³No, ²⁵⁹Fm, ²⁵⁵Cf, ^247,251Bk, ²⁴³Am, ²³⁹Pu, ²³⁵Np(α); ²⁵¹Cm, ²⁴⁷Am, ²³⁹Np, ²³⁵U(β^-); predicted decay chains of ²⁸³Cn (Z=112), ²⁹¹Lv (Z=116), ²⁹⁵Og (Z=118), ²⁹⁶119 (Z=119), and ²⁹⁹120 (Z=120).

doi: 10.1103/PhysRevC.102.064605
Citations: PlumX Metrics

2020SR01      Nucl.Phys. A995, 121689 (2020)

M.G.Srinivas, H.C.Manjunatha, K.N.Sridhar, N.Sowmya, A.Cecil Raj

Proton decay of actinide nuclei

doi: 10.1016/j.nuclphysa.2019.121689
Citations: PlumX Metrics

2019MA01      Nucl.Phys. A981, 17 (2019)

H.C.Manjunatha, K.N.Sridhar, H.B.Ramalingam

Synthesis of superheavy elements using ^{50, 51}V-induced fusion reactions

NUCLEAR STRUCTURE ¹⁶⁸Ta; calculated proton, neutron sp levels near Fermi surface, energy, J, π, occupation probability of orbitals, kinematic high spin rotational bands, band crossings, moment of inertia, major shells using PNC-CSM (Particle Number Conserving) method - Cranking Shell Model. High-spin rotational bands compared to data.

doi: 10.1016/j.nuclphysa.2018.10.084
Citations: PlumX Metrics

2019MA39      Nucl.Phys. A987, 382 (2019)

H.C.Manjunatha, K.N.Sridhar, N.Sowmya

Investigations on ⁶⁴Ni + _ZAn^A → _Z=104-123(SHN)^A=250-310

NUCLEAR REACTIONS ¹⁹²Os, ¹⁹³Ir, ^194,195,196Pt, ^197,198Au, ²⁰²Hg, ^204,205Tl, ^207,208Pb, ²⁰⁹Bi, ²⁰⁹Po, ^223,226Ra, ^225,227Ac, ^230,232Th, ²³¹Pa, ^232,238U, ^235,237Np, ²³⁹Pu, ^241,243Am(⁶⁴Ni, x), E^*=35 MeV;(⁶⁴Ni, xn), E^*=20-45 MeV; calculated compound nucleus formation probability and yields of superheavies for Ni projectiles, evaporation residue elements σ_ER for x=3, 4 and 5; identified suitable targets for synthesis of superheavy elements using ⁶⁴Ni fusion reactions.

doi: 10.1016/j.nuclphysa.2019.05.006
Citations: PlumX Metrics

2019MA86      Phys.Part. and Nucl.Lett. 16, 647 (2019)

H.C.Manjunatha, K.N.Sridhar

A Detail Investigation on the Synthesis of Superheavy Element Z = 119

doi: 10.1134/s1547477119060487
Citations: PlumX Metrics

2019SR01      Nucl.Phys. A983, 195 (2019)

K.N.Sridhar, H.C.Manjunatha, H.B.Ramalingam

Studies on the synthesis superheavy element Z = 120

RADIOACTIVITY ^{290,291,292,293,294,295,296,297,298,299,300,301,302,303,304}120 (SF), (α); calculated T_1/2 of both α-decay and spontaneous fission using Coulomb potential plus proximity potential; calculated decay chains and maximum evaporation residue σ for different projectile-target combinations, proper E^* and different neutron evaporation channels to achieve maximal σ; deduced superheavy σ, most probable projectile-target combination to synthetize superheavy Z=120 is Ti+Cf. Halflives and σ compared to available data.

doi: 10.1016/j.nuclphysa.2018.11.032
Citations: PlumX Metrics

2019SR04      Pramana 93, 81 (2019)

G.R.Sridhara, H.C.Manjunatha, K.N.Sridhar, H.B.Ramalingam

Systematic study of the α decay properties of actinides

RADIOACTIVITY ^{211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238}Ac, ^{214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236}Th, ^{217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240}Pa, ^{219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245}U, ^{221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245}Np, ^{228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245}Pu, ^{228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250}Am, ^{233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250,251}Cm, ²⁵⁵Cm, ^{234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250,251,252}Bk, ^{238,239,240,241,242,243,244,245,246,247,248,249,250,251,252,253,254,255}Cf, ^{241,242,243,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258}Es, ^{243,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258}Fm, ^{246,247,248,249,250,251,252,253,254,255,256,257,258,259}Md, ^{246,247,248,249,250,251,252,253,254,255,256,257,258,259,260}No, ^{251,252,253,254,255,256,257,258,259,260,261,262}Lr(α); calculated T_1/2. Comparison with available data.

RADIOACTIVITY ²¹⁰Ac, ^{200,201,202,203,204,205,206,207,208,209,210,211,212,213}Th, ^{200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216}Pa, ^{210,211,212,213,214,215,216,217,218}U, ^{215,216,217,218,219,220}Np, ^{220,221,222,223,224,225,226,227}Pu, ^226,227Am, ^252,253,254Cm, ^{230,231,232,233}Bk, ^253,254,255Bk, ^{230,231,232,233,234,235,236,237}Cf, ^{235,236,237,238,239,240}Es, ^259,260Es, ^{235,236,237,238,239,240,241,242}Fm, ^259,260Fm, ^{240,241,242,243,244,245}Md, ²⁶⁰Md, ²⁴⁵No, ^{261,262,263,264,265}No, ^{245,246,247,248,249,250}Lr, ^263,264,265Lr(SF); calculated T_1/2. Comparison with available data.

doi: 10.1007/s12043-019-1845-9
Citations: PlumX Metrics

2018MA19      Nucl.Phys. A971, 83 (2018)

H.C.Manjunatha, K.N.Sridhar

Fusion barrier characteristics of actinides

NUCLEAR STRUCTURE Z=89-103; calculated fusion barrier parameters (position, height, width) by using data of more than 7000 different combinations of projectile and target leading to the same composite system; deduced parameters, fusion σ formula. Compared with other parameterizations and with data.

doi: 10.1016/j.nuclphysa.2018.01.016
Citations: PlumX Metrics

2018MA31      Nucl.Phys. A975, 136 (2018)

H.C.Manjunatha, K.N.Sridhar

Investigation to synthesis more isotopes of superheavy nuclei Z=118

RADIOACTIVITY ^{291,293,295,297,299,301}Og(α); calculated T_1/2, α-decay chains (ending with Og(SF) nuclei).

NUCLEAR REACTIONS Cf(Ca, x), Cm(Ti, x), Bk(Sc, x), Am(V, x), Pu(Cr, x), U(Fe, x), Np(Mn, x), Th(Ni, x), Pb(Kr, x); calculated simple relations for maximum evapopration residue σ and the corresponding energy, reaction Q-values, nucleon separation energy, fusion barriers, evaporation residue σ vs projectile mass number, maximum evaporation σ, compound nucleus formation probability, survival probability, α-decay chains (ending with Og(SF) nuclei); deduced parameters.

doi: 10.1016/j.nuclphysa.2018.04.009
Citations: PlumX Metrics

2018MA50      Phys.Rev. C 98, 024308 (2018)

H.C.Manjunatha, K.N.Sridhar, N.Sowmya

Investigations of the synthesis of the superheavy element Z=122

NUCLEAR REACTIONS ²⁵⁰Cm(⁵⁷Fe, X)³⁰⁷122^*, E(cm)=288 MeV; ²⁴⁷Cm(⁶⁰Fe, X)³⁰⁷122^*, E(cm)=287 MeV; ²⁴⁴Pu(⁶³Ni, X)³⁰⁷122^*, E(cm)=302 MeV; ²³⁵U(⁷²Zn, X)³⁰⁷122^*, E(cm)=314 MeV; ²²⁸Ra(⁷⁹Se, X)³⁰⁷122^*, E(cm)=339 MeV; ²⁵⁰Cm(⁵⁸Fe, X)³⁰⁸122^*, E(cm)=284 MeV; ²⁴⁸Cm(⁶⁰Fe, X)³⁰⁸122^*, E(cm)=283 MeV; ²⁴⁴Pu(⁶⁴Ni, X)³⁰⁸122^*, E(cm)=297 MeV; ²³⁸U(⁷⁰Zn, X)³⁰⁸122^*, E(cm)=310 MeV; ²³⁶U(⁷²Zn, X)³⁰⁸122^*, E(cm)=310 MeV; ²³²Th(⁷⁶Ge, X)³⁰⁸122^*, E(cm)=322 MeV; ²²⁸Ra(⁸⁰Se, X)³⁰⁸122^*, E(cm)=334 MeV; ²²⁶Ra(⁸²Se, X)³⁰⁸122^*, E(cm)=334 MeV; ²⁵⁶Cf(⁵³Cr, X)³⁰⁹122^*, E(cm)=266 MeV; ²⁵⁵Cf(⁵⁴Cr, X)³⁰⁹122^*, E(cm)=266 MeV; ²⁵²Cm(⁵⁷Fe, X)³⁰⁹122^*, E(cm)=281 MeV; ²⁵¹Cm(⁵⁸Fe, X)³⁰⁹122^*, E(cm)=281 MeV; ²⁵⁰Cm(⁵⁹Fe, X)³⁰⁹122^*, E(cm)=281 MeV; ²⁴⁹Cm(⁶⁰Fe, X)³⁰⁹122^*, E(cm)=280 MeV; ²⁴³Pu(⁶⁶Ni, X)³⁰⁹122^*, E(cm)=294 MeV; ²³⁹U(⁷⁰Zn, X)³⁰⁹122^*, E(cm)=308 MeV; ²³⁷U(⁷²Fe, X)³⁰⁹122^*, E(cm)=307 MeV; ²³³Th(⁷⁶Ge, X)³⁰⁹122^*, E(cm)=320 MeV; ²³⁰Ra(⁷⁹Se, X)³⁰⁹122^*, E(cm)=332 MeV; ²²⁷Ra(⁸²Se, X)³⁰⁹122^*, E(cm)=331 MeV; ²⁵⁶Cf(⁵⁴Cr, X)³¹⁰122^*, E(cm)=263 MeV; ²⁵²Cm(⁵⁸Fe, X)³¹⁰122^*, E(cm)=278 MeV; ²⁵¹Cm(⁵⁹Fe, X)³¹⁰122^*, E(cm)=278 MeV; ²⁵⁰Cm(⁶⁰Fe, X)³¹⁰122^*, E(cm)=278 MeV; ²⁴⁴Pu(⁶⁶Ni, X)³¹⁰122^*, E(cm)=291 MeV; ²³⁸U(⁷²Zn, X)³¹⁰122^*, E(cm)=304 MeV; ²³⁴Th(⁷⁶Ge, X)³¹⁰122^*, E(cm)=317 MeV; ²³⁵Ac(⁷⁵As, X)³¹⁰122^*, E(cm)=324 MeV; ²³⁰Ra(⁸⁰Se, X)³¹⁰122^*, E(cm)=329 MeV; ²²⁸Ra(⁸²Se, X)³¹⁰122^*, E(cm)=328 MeV; (⁶⁰Fe, X)³¹¹122^*, E(cm)=277 MeV; ²³⁹U(⁷²Zn, X)³¹¹122^*, E(cm)=303 MeV; ²³⁶Ac(⁷⁵As, X)³¹¹122^*, E(cm)=323 MeV; ²³⁵Ac(⁷⁶As, X)³¹¹122^*, E(cm)=323 MeV; ²³⁴Ac(⁷⁷As, X)³¹¹122^*, E(cm)=322 MeV; ²³⁴Ra(⁷⁷Se, X)³¹¹122^*, E(cm)=329 MeV; ²³³Ra(⁷⁸Se, X)³¹¹122^*, E(cm)=328 MeV; ²³²Ra(⁷⁹Se, X)³¹¹122^*, E(cm)=328 MeV; ²³¹Ra(⁸⁰Se, X)³¹¹122^*, E(cm)=328 MeV; ²²⁹Ra(⁸²Se, X)³¹¹122^*, E(cm)=327 MeV; ²⁵²Cm(⁶⁰Fe, X)³¹²122^*, E(cm)=277 MeV; ²³⁶Ac(⁷⁶As, X)³¹²122^*, E(cm)=322 MeV; ²³⁵Ac(⁷⁷As, X)³¹²122^*, E(cm)=322 MeV; ²³⁴Ra(⁷⁸Se, X)³¹²122^*, E(cm)=328 MeV; ²³³Ra(⁷⁹Se, X)³¹²122^*, E(cm)=328 MeV; ²³²Ra(⁸⁰Se, X)³¹²122^*, E(cm)=328 MeV; ²³⁰Ra(⁸²Se, X)³¹²122^*, E(cm)=327 MeV; ²³⁶Ac(⁷⁷As, X)³¹³122^*, E(cm)=322 MeV; ²³⁴Ra(⁷⁹Se, X)³¹³122^*, E(cm)=328 MeV; ²³³Ra(⁸⁰Se, X)³¹³122^*, E(cm)=327 MeV; ²³¹Ra(⁸²Se, X)³¹³122^*, E(cm)=327 MeV; ²³⁴Ra(⁸⁰Se, X)³¹⁴122^*, E(cm)=327 MeV; ²³²Ra(⁸²Se, X)³¹⁴122^*, E(cm)=326 MeV; calculated evaporation residue σ, compound nucleus formation probability, and survival probability. Dinuclear system (DNS) model. Discussed most probable projectile-target combinations to synthesize the superheavy element Z=122.

RADIOACTIVITY ^{307,308,309,310,311,312,313,314}122(α), (¹²C), (¹⁴C), (¹⁴N), (²⁰Ne), (²²Ne), (²⁴Ne), (²⁸Si), (³⁰Si), (³²Si), (³⁴Si), (³⁶Ar), (³⁸Ar), (⁴⁰Ar), (⁴²Ar), (⁴⁴Ar), (⁴⁰Ca), (⁴²Ca), (⁴⁴Ca), (⁴⁶Ca), (⁴⁸Ca), (SF); calculated half-lives, Q values, penetrability, branching ratios relative to α decay. Dinuclear system (DNS) model.

doi: 10.1103/PhysRevC.98.024308
Citations: PlumX Metrics

2018SR05      Phys.Rev. C 98, 064605 (2018)

K.N.Sridhar, H.C.Manjunatha, H.B.Ramalingam

Search for possible fusion reactions to synthesize the superheavy element Z=121

RADIOACTIVITY ^{299,300,301,302,303,304,305}121, ^{295,296,297,298,299,300}119, ^{291,292,293,294,295,296}Ts, ^287,288,289Mc(α), (SF); calculated half-lives for different decay modes using Wong model for SF decay. Comparison with several other theoretical calculations.

NUCLEAR STRUCTURE ^{280,281,282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320,321,322,323,324,325,326,327,328,329,330}121; calculated S(n), S(p), S(2n), S(2p), Q(β).

NUCLEAR REACTIONS ^249,250,251Cf(⁵⁰V, 2n), ^250,252Cf(⁵¹V, 2n), ²⁴⁴Pu(⁶⁰Co, 2n)³⁰²121, ²⁵⁰Cm(⁵⁵Mn, 2n)³⁰³121, E^*=20-50 MeV; calculated evaporation σ(E). ^{299,300,301,302,303,304,305}121; calculated compound nucleus probability, and survival probability at 35 MeV excitation energy and 2n channel reaction as a function of projectile mass number. ^{249,250,251,252,253,254}Cf(⁴⁸V, xn), (⁴⁹V, xn), (⁵⁰V, xn), (⁵¹V, xn), E^*=20, 25, 30, 35 MeV; ^247,248,249Bk(⁵⁰Cr, xn), (⁵¹Cr, xn), (⁵²Cr, xn), (⁵³Cr, xn), (⁵⁴Cr, xn), E^*=20, 25, 30, 35 MeV; ^{244,245,246,247,248,250}Cm(⁵²Mn, xn), (⁵³Mn, xn), (⁵⁴Mn, xn), (⁵⁵Mn, xn), E^*=20, 25, 30, 35 MeV; ^241,242,243Am(⁵⁶Fe, xn), (⁵⁷Fe, xn), (⁵⁸Fe, xn), (⁶⁰Fe, xn), E^*=20, 25, 30, 35 MeV; ^{239,240,241,242,244}Pu(⁵⁹Co, xn), (⁶⁰Co, xn), E^*=15-35 MeV, x=1-6. calculated evaporation residue σ(E) for the production of ^{300,301,302,303,304,305}121 nuclei, fusion barrier heights.

doi: 10.1103/PhysRevC.98.064605
Citations: PlumX Metrics

2017MA20      Nucl.Phys. A962, 7 (2017)

H.C.Manjunatha, K.N.Sridhar

Projectile target combination to synthesis superheavy nuclei Z=126

NUCLEAR STRUCTURE ^{307,318,319,320}126; calculated different combinations of colliding ions with varied energy capable to reach isotopes of Z=126 element, their fusion, fission, survival σ, compound nucleus formation and survival probability, α-decay chains (finishing at spontaneously fissioning isotopes of Hs, Lv and Og); deduced, identified most probable combination of nuclei and energy.

doi: 10.1016/j.nuclphysa.2017.03.007
Citations: PlumX Metrics

2017MA25      Eur.Phys.J. A 53, 97 (2017)

H.C.Manjunatha, K.N.Sridhar

Survival and compound nucleus probability of super heavy element Z = 117

NUCLEAR STRUCTURE ^{289,290,291,292,293,294,295,296,297}Ts; calculated possible projectile-target combinations for Ts synthesis, where the driving potential has its minimum, fusion σ, survival σ, fission σ.

NUCLEAR REACTIONS ²³⁸U, ^242,243Pu, ²⁴³Am, ^245,248Cm, ²⁴⁹Bk, ²⁹⁴Cf(⁴⁸Ca, xn), E^*=31-53 MeV; calculated evaporation residue σ leading to Z=112-117. ²⁰³Tl(⁸⁶Kr, xn), ²¹³Bi(⁸⁰Se, xn), ²²²At(⁷⁴Ge, xn), ²²³Fr(⁷⁰Zn, xn), ²³²Ra(⁶⁵Cu, xn), ²³²Ac(⁶⁴Ni, xn), ²⁴⁹Bk(⁸⁰Se, xn), ^259,260Md(³⁶S, xn), E(cm)=180-360 MeV; calculated evaporation residue σ leading on Ts isotopes; deduced suitable ways to synthetize Ts element.

doi: 10.1140/epja/i2017-12279-4
Citations: PlumX Metrics

2017MA42      Eur.Phys.J. A 53, 156 (2017)

H.C.Manjunatha, K.N.Sridhar

New semi-empirical formula for α-decay half-lives of the heavy and superheavy nuclei

RADIOACTIVITY Z=95-135(α); calculated T_1/2 of isotopes of given nuclei (separately for even and odd Z) vs A/√; deduced parameters for newly suggested formula using fit to data of more than 2600 isotopes.

doi: 10.1140/epja/i2017-12337-y
Citations: PlumX Metrics

2017MA78      Eur.Phys.J. A 53, 196 (2017)

H.C.Manjunatha, K.N.Sridhar

A probability of synthesis of the superheavy element Z=124

NUCLEAR STRUCTURE ^{313,314,315,316,317,318}124; calculated total fusion σ, survival probability, evaporation residue σ vs E(cm) for combinations of different isotopes Cm+Ni, Bk+Co, Cf+Fe, Pu+Zn, Ac+Br, Th+Se, U+Ge, Ra+Kr, Ac+Br, Th+Se, U+Ge, Pu+Zn, Rn+Sr, At+Y giving the composite system at excitation energy E^*=0-95 MeV; deduced projectile-target combinations with maximal fusion σ, combinations with maximum survival σ and minimal fission σ.

doi: 10.1140/epja/i2017-12380-8
Citations: PlumX Metrics

1999MA32      Phys.Rev. D60, 014009 (1999)

P.Mathews, K.Sridhar, R.Basu

J/ψ + γ Production at the CERN LHC

doi: 10.1103/PhysRevD.60.014009
Citations: PlumX Metrics

1998MA68      Phys.Lett. 438B, 336 (1998); Erratum Phys.Lett. 450B, 479 (1999)

P.Mathews, P.Poulose, K.Sridhar

η_c Production at the Tevatron: A test of NRQCD

NUCLEAR REACTIONS ¹H(p-bar, X), E(cm)=1.8 TeV; calculated η(c) production σ(pT). Testable NRQCD prediction.

doi: 10.1016/S0370-2693(98)00990-3
Citations: PlumX Metrics

1998SR03      Phys.Lett. 438B, 211 (1998)

K.Sridhar, A.D.Martin, W.J.Stirling

J/ψ Production at the Tevatron and HERA: The effect of k_T Smearing

NUCLEAR REACTIONS ¹H(p-bar, X), E(cm)=1.8 TeV; ¹H(γ, X), E(cm)=100 GeV; analyzed J/ψ production data; deduced k(T) smearing effects, role in NRQCD tests.

doi: 10.1016/S0370-2693(98)00956-3
Citations: PlumX Metrics

1994LE32      Nucl.Phys. B419, 3 (1994)

E.Leader, K.Sridhar

γ(*), Z(*) Production in Polarized pp Scattering as a Probe of the Proton Spin Structure

NUCLEAR REACTIONS ¹H(p, X), E=Collider energies; calculated Drell-Yan process σ.

doi: 10.1016/0550-3213(94)90354-9
Citations: PlumX Metrics

Note: The following list of authors and aliases matches the search parameter K.Sridhar: , K.N.SRIDHAR