Skip navigation

Browsing by Author Gothe D.A.

Jump to: 0-9 A B C D E F G H I J K L M N O P Q R S T U V W X Y Z
or enter first few letters:  
Showing results 1 to 11 of 11
Issue DateTitleAuthor(s)
2010A LaBr3:Ce-NaI(Tl) Phoswich for X- and low energy γ-ray astronomyMazumdar I.; Anil Kumar, G.; Gothe D.A.; Manchanda R.K.
2013Effect of angular momentum on giant dipole resonance observables in the 28Si+116Cd reactionMukul I.; Roy A.; Sugathan P.; Gehlot J.; Mohanto G.; Madhavan N.; Nath S.; Dubey R.; Mazumdar I.; Gothe D.A.; Kaur M.; Kumar A.K.R.; Arumugam, Paramasivan
2009Efficiency calibration and coincidence summing correction for large arrays of NaI(Tl) detectors in soccer-ball and castle geometriesAnil Kumar, G.; Mazumdar I.; Gothe D.A.
2009Efficiency calibration and simulation of a LaBr3(Ce) detector in close-geometryAnil Kumar, G.; Mazumdar I.; Gothe D.A.
2009Experimental measurements and GEANT4 simulations for a comparative study of efficiencies of LaBr3:Ce, NaI(Tl), and BaF2Anil Kumar, G.; Mazumdar I.; Gothe D.A.
2008GEANT4 simulation of a new 4π sum-spin spectrometer at TIFRAnil Kumar, G.; Mazumdar I.; Gothe D.A.
2013Giant dipole resonance in A ∼ 144 mass regionMukul I.; Sugathan P.; Mazumdar I.; Gehlot J.; Mohanto G.; Kaur M.; Rhine Kumar A.K.; Madhavan N.; Nath S.; Dubey R.; Gothe D.A.; Arumugam, Paramasivan; Roy A.
2009Search for rare shape transition and gqr decay in hot rotating 188Os nucleusMazumdar I.; Gothe D.A.; Anil Kumar, G.; Aggarwal M.; Joshi P.K.; Palit R.; Jain H.C.
2011Shape transition and isovector giant quadrupole resonance decay in hot rotating nucleiMazumdar I.; Gothe D.A.; Anil Kumar, G.; Aggarwal M.
2015Spin gated GDR widths at moderate temperaturesMukul I.; Sugathan P.; Gehlot J.; Mohanto G.; Rhine Kumar A.K.; Mazumdar I.; Kaur M.; Madhavan N.; Nath S.; Dubey R.; Banerjee T.; Saneesh N.; Gothe D.A.; Arumugam, Paramasivan; Roy A.; Madhavan N.; Navin A.; Rehm K.E.; Hinde D.J.; Simenel C.; Gomes P.R.S.
2013Studying the properties and response of a large volume (946 cm3) LaBr3:Ce detector with γ-rays up to 22.5 MeVMazumdar I.; Gothe D.A.; Anil Kumar, G.; Yadav N.; Chavan P.B.; Patel S.M.