output
20022025
most citedFlavour physics of leptons and dipole moments

378 citations

Showing 2016Show all

33 papers · 1 filter

hep-ph201644 cited

Improved limits on the hadronic and semi-hadronic CP violating parameters and role of a dark force carrier in the electric dipole moment of Hg

B. K. Sahoo

Combining the recently reported electric dipole moment (EDM) of Hg atom due to breaking of parity and time-reversal symmetries with the improved relativistic atomic calcula…

physics.atom-ph201610 cited

RCCPAC: A parallel relativistic coupled-cluster program for closed-shell and one-valence atoms and ions in FORTRAN

B. K. Mani, Siddhartha Chattopadhyay, D. Angom

We report the development of a parallel FORTRAN code, RCCPAC, to solve the relativistic coupled-cluster equations for closed-shell and one-valence atoms and ions. The parallelizati…

astro-ph.SR201629 cited

Rise and fall of the dust shell of the classical nova V339 Delphini

A. Evans, D. P. K. Banerjee, R. D. Gehrz +16

We present infrared spectroscopy of the classical nova V339 Delphini, obtained over a year period. The infrared emission lines were initially symmetrical, with HWHM velocit…

astro-ph.GA201649 cited

Search for Interstellar monohydric Thiols

Prasanta Gorai, Ankan Das, Amaresh Das +3

It has been pointed out by various astronomers that very interesting relationship exists between interstellar alcohols and the corresponding thiols (sulfur analogue of alcohols) as…

cond-mat.mtrl-sci201624 cited

Qualitative observation of reversible phase change in astrochemical ethanethiol ices using infrared spectroscopy

S Pavithraa, R Rajan, P Gorai +7

Here we report the first evidence for a reversible phase change in an ethanethiol ice prepared under astrochemical conditions. InfraRed (IR) spectroscopy was used to monitor the mo…

astro-ph.SR201623 cited

Amplitude of solar wind density turbulence from 10--45

K. Sasikumar Raja, Madhusudan Ingale, R. Ramesh +3

We report on the amplitude of the density turbulence spectrum () and the density modulation index () in the solar wind between and . We derive t…