Chandradew Sharma
Yonsei University
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Featured researches published by Chandradew Sharma.
Physical Review D | 2008
Rahul Basu; P. N. Pandita; Chandradew Sharma
We study the production of the lightest neutralinos in the radiative process e{sup +}e{sup -}{yields}{chi}-tilde{sub 1}{sup 0}{chi}-tilde{sub 1}{sup 0}{gamma} in low energy supersymmetric models for the International Linear Collider energies. This includes the minimal supersymmetric standard model as well as its extension with an additional chiral Higgs singlet superfield, the nonminimal supersymmetric standard model. We compare and contrast the dependence of the signal cross section on the parameters of the neutralino sector of the minimal and nonminimal supersymmetric standard model. We also consider the background to this process coming from the standard model process e{sup +}e{sup -}{yields}{nu}{nu}{gamma}, as well as from the radiative production of the scalar partners of the neutrinos (sneutrinos) e{sup +}e{sup -}{yields}{nu}-tilde{nu}-tilde*{gamma}, which can be a background to the radiative neutralino production when the sneutrinos decay invisibly. In low energy supersymmetric models radiative production of the lightest neutralinos may be the only channel to study supersymmetric partners of the standard model particles at the first stage of a linear collider, since heavier neutralinos, charginos, and sleptons may be too heavy to be pair produced at a e{sup +}e{sup -} machine with {radical}(s)=500 GeV.
Physics Letters B | 2007
Maxime Imbeault; David London; Chandradew Sharma; Nita Sinha; Rahul Sinha
Abstract We show that any new physics (NP) which affects B decays with penguin contributions can be absorbed by redefinitions of the Standard Model (SM) diagrammatic amplitudes. Hence, there are no signals of NP in such decays unless there is an accurate theoretical estimate of hadronic parameters or a justifiable approximation can be made. In all decays with penguin contributions, NP simultaneously affects pairs of diagrams. The evidence for a large C ′ from fits to B → π K data is naturally explained if NP contributes to P EW ′ , since NP affects the P EW ′ and C ′ diagrams as a pair. The weak phase γ measured in B → π K decays will always agree with its SM value even in the presence of NP, if the NP contributes in such a way that the amplitudes retain the SM form after suitable redefinitions.
Physical Review D | 2006
Chandradew Sharma; Rahul Sinha
The analysis of
Physical Review D | 2005
Chandradew Sharma; Rahul Sinha
B \to \jpsi K^{\star}_{2}(1430)
Physica A-statistical Mechanics and Its Applications | 2015
Chandradew Sharma; Kinjal Banerjee
decay mode is complicated by the fact that close to the
Physical Review D | 2012
P. N. Pandita; Chandradew Sharma
J^{PC}=2^{++}
Physical Review Letters | 2011
Rahul Sinha; Nilendra G. Deshpande; Sandip Pakvasa; Chandradew Sharma
meson
International Journal of Modern Physics B | 2017
Kinjal Banerjee; Chandradew Sharma; N. Bittu
\Kstart(1430)
International Journal of Modern Physics A | 2008
C. S. Kim; Sechul Oh; Chandradew Sharma; Rahul Sinha; Yeo Woong Yoon
, there lie other
Physical Review D | 2007
C. S. Kim; Sechul Oh; Chandradew Sharma; Rahul Sinha; Yeo Woong Yoon
J^{PC}=1^{--}