Physics – Condensed Matter – Strongly Correlated Electrons
Scientist
Physics
Condensed Matter
Strongly Correlated Electrons
Scientist
Inter University Accelerator Centre, New Delhi
Atmospheric Research Laboratory, Physics Department, Banaras Hindu University, Varanasi-221005, India Hindu University, Varanasi, India
V.K.S. University, Ara, Bihar, India
National Physical Laboratory, New Delhi, India
Department of Physics, Banaras Hindu University, Varanasi-221 005, India
Atmospheric Physics Lab., Physics Department, Banaras Hindu University, Varanasi-221005, India Research Laboratory, Physics Department, Banaras Hindu University, Varanasi-221005, India Research Lab., Department of Physics, Banaras Hindu University
Atmospheric Research Laboratory, Department of Physics, B.H.U.
Department of Physics, Banaras Hindu University, Varanasi 211 005, India
Atmospheric Research Laboratory, Physics Department, Banaras Hindu University, Varanasi, 221 005, India, INGeophysical Department, Eötvös University, Budapest, Pf. 32, H-1532, Hungary, HU
Physics Department, Banaras Hindu University, Varanasi-221005, India
Atmospheric Research Lab., Physics Department, Banaras Hindu University
Atmospheric Research Laboratory, Physics Department, Banaras Hindu University, Varanasi 221005, India V.K.S. University, Ara, Bihar, India
Department of Physics, Banaras Hindu University, Varanasi 221 005, India
Space Physics Laboratory, Physics Department, B.H.U., Varanasi 221005, India
Inter University Accelerator Centre, Aruna Asaf Ali Marg, Delhi-110067, India
Department of Physics, Banaras Hindu University, Varanasi-211 005, India
Department of Civil Engineering, Indian Institute of Technology, Kanpur-208 016, India
Indian Inst. of Technology, Kanpur, India
Physics Department, Banaras Hindu University, Varanasi - 221 005, India
Atmospheric Research Laboratory, Physics Department, Banaras Hindu University
Center for Earth Observing and Space Research, School of Computational Sci
A case study of whistlers recorded at Varanasi (L = 1.07)
A New Class of Inhomogeneous String Cosmological Models in General Relativity
A theoretical verification of intensity of plasmaspheric ELF hiss emissions: theory versus GEOS-1 observations
Absence of M2 Retardation in $^{35}Cl$: Evidence for Stronger Isospin-Mixing Effects in A=35 Mirror Nuclei
Amplification of signal by Cerenkov resonance interaction
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