B
B. S. Nara Singh
Researcher at University of the West of Scotland
Publications - 92
Citations - 1051
B. S. Nara Singh is an academic researcher from University of the West of Scotland. The author has contributed to research in topics: Excited state & Neutron. The author has an hindex of 14, co-authored 79 publications receiving 869 citations. Previous affiliations of B. S. Nara Singh include Tata Institute of Fundamental Research & Weizmann Institute of Science.
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Journal ArticleDOI
Evidence for a spin-aligned neutron–proton paired phase from the level structure of 92Pd
Bo Cederwall,F. Ghazi Moradi,Torbjörn Bäck,A. Johnson,J. Blomqvist,E. Clément,R. Wadsworth,K. Andgren,Karin Lagergren,Karin Lagergren,A. Dijon,G. Jaworski,G. Jaworski,Roberto Liotta,Chong Qi,B. M. Nyakó,Johan Nyberg,M. Palacz,H. Al-Azri,Alejandro Algora,G. de Angelis,A. Atac,S. Bhattacharyya,S. Bhattacharyya,Tina Penick Brock,J. R. Brown,P. J. Davies,A. Di Nitto,Zs. Dombrádi,A. Gadea,J. Gal,Baharak Hadinia,F. Johnston-Theasby,Pankaj S. Joshi,K. Juhasz,R. Julin,A. Jungclaus,Gábor Kalinka,S. O. Kara,Anton Khaplanov,J. Kownacki,G. La Rana,S. M. Lenzi,Jozsef Molnar,R. Moro,D. R. Napoli,B. S. Nara Singh,A. Persson,F. Recchia,M. Sandzelius,M. Sandzelius,J. N. Scheurer,G. Sletten,Dóra Sohler,Pär-Anders Söderström,Michael Taylor,J. Timár,J. J. Valiente-Dobon,E. Vardaci,S. Williams +59 more
TL;DR: It is suggested that this coupling scheme replaces normal superfluidity in the ground and low-lying excited states of the heaviest N = Z nuclei, and has a considerable impact on the nuclear level structure and possibly influence the dynamics of rapid proton capture in stellar nucleosynthesis.
Journal ArticleDOI
New precision measurement of the 3He(4He,gamma) 7Be cross section.
TL;DR: The 3He(4He,gamma) 7Be reaction plays an important role in determining the high energy solar neutrino flux and in understanding the abundances of primordial 7Li.
Journal ArticleDOI
Shell Erosion and Shape Coexistence in (16)43S27.
L. Gaudefroy,J. M. Daugas,Michael Hass,S. Grévy,Ch. Stodel,J. C. Thomas,L. Perrot,Michel Girod,B. Rossé,J. C. Angélique,D. L. Balabanski,E. Fiori,C. Force,Georgi P. Georgiev,D. Kameda,V. Kumar,R. Lozeva,I. Matea,I. Matea,V. Méot,P. Morel,B. S. Nara Singh,F. Nowacki,G. S. Simpson +23 more
TL;DR: In this article, the first isomeric state in {sub 16}{sup 43}S{sub 27}[E{sub x}=320.5(5) keV, T{sub 1/2}=415(5] ns, and g=0.317(4)].
Journal ArticleDOI
Evidence for a smooth onset of deformation in the neutron-rich Kr isotopes
M. Albers,N. Warr,Kosuke Nomura,A. Blazhev,J. Jolie,D. Mücher,B. Bastin,C. Bauer,C. Bernards,L. Bettermann,Vinzenz Bildstein,Jonathan Butterworth,M. Cappellazzo,Joakim Cederkäll,D. Cline,Iain Darby,S. Das Gupta,J. M. Daugas,Thomas Davinson,H. De Witte,Jan Diriken,D. M. Filipescu,E. Fiori,C. Fransen,Liam Gaffney,Georgi P. Georgiev,R. Gernhäuser,M. Hackstein,Stefan Heinze,Herbert Hess,Mark Huyse,D. G. Jenkins,Joonas Konki,M. Kowalczyk,T. Kröll,R. Krücken,J. Litzinger,R. Lutter,N. Marginean,C. Mihai,K. Moschner,P. J. Napiorkowski,B. S. Nara Singh,K. Nowak,Takaharu Otsuka,Janne Pakarinen,M. Pfeiffer,D. Radeck,P. Reiter,Susan Rigby,L. M. Robledo,R. R. Rodríguez-Guzmán,M. Rudigier,Pedro Sarriguren,Marcus Scheck,M. Seidlitz,B. Siebeck,G. S. Simpson,P. Thöle,T. Thomas,J. Van de Walle,P. Van Duppen,M. Vermeulen,D. Voulot,R. Wadsworth,Fredrik Wenander,Kathrin Wimmer,K. O. Zell,M. Zielinska +68 more
TL;DR: In this article, the level energies of the first excited 2(+) states and their absolute E2 transition strengths to the ground state were determined and discussed in the context of the E(2(1+)) and B(E2;2( 1+)-> 0(1)(+)) systematics of the krypton chain.
Journal ArticleDOI
40Ca(alpha, gamma)44Ti reaction in the energy regime of supernova nucleosynthesis.
Hisham Nassar,Michael Paul,I. Ahmad,Y. Ben-Dov,J. Caggiano,S. Ghelberg,S. Goriely,John P. Greene,Michael Hass,Alexander Heger,Alexander Heger,A. M. Heinz,D. J. Henderson,R. V. F. Janssens,C. L. Jiang,Y. Kashiv,B. S. Nara Singh,Avishai Ofan,R. C. Pardo,T. Pennington,K. E. Rehm,Guy Savard,R. Scott,R. C. Vondrasek +23 more
TL;DR: In this article, the authors investigated in the laboratory the major {sup 44}Ti production reaction {sup 40}Ca({alpha},{gamma}), and showed that the associated stellar rate has important astrophysical consequences, increasing the calculated supernova {sup 42}Ti yield by a factor {approx 2 over previous estimates and bringing it closer to Cas A observations.