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Ramanath Cowsik
Courses Research Interests He has studied the virial discrepancy in the dynamics of clusters of galaxies and proposed the idea of weakly interacting particles as constituting the 'dark matter' that is responsible for the formation and the gravitational binding of galaxies and clusters of galaxies. Assuming thermodynamic equilibrium in the early hot and condensed state of a big-bang Universe, he calculated precisely the number density of the relict neutrinos, and thence derived a strict upper bound on the masses of the neutrinos - the 'Cowsik-McClelland bound'. His work, especially in the area of cosmology, is interdisciplinary in character and connects laboratory Physics with the large scale phenomena of the Universe. Accordingly, he has set useful bounds on the radiative instability of neutrinos and on baryon number, non-conserving proton-decay and neutron-antineutron oscillations. He developed a new method of deriving the age of the Universe from studies of the isotopic anomalies in pre-solar grains of aluminum oxide found in meteorites. Non-accelerator particle physics refers to the study of fundamental particles and their interactions without using huge accelerators like FermiLab. Cowsik performed the first detailed calculations on the fluxes of neutrinos generated by cosmic-ray interactions in the atmosphere and discussed their observation in detectors placed deep underground--a study that later led to the discovery of neutrino oscillations at Kamiokande in Japan. At the Washington University, he and his colleagues measured the longest radioactive half-life ever, of the double beta decay of Te-128, as 7.7 x 1024 years. This long lifetime, in conjunction with the shorter lifetime of Te-130, implies an upper bound of ~1 eV on the Majorana mass of the neutrino, and strict bounds on majoran couplings. Most recently with a highly sensitive torsion balance he and his students have successfully observed the 'finite temperature' corrections to the Casimir forces which come into play at large separations. His current efforts are primarily directed towards building an extremely sensitive torsion balance to probe possible violations of the inverse square law of gravity at sub-millimeter scales that are predicted by 'string-motivated' theories. This is a follow up of his longstanding interest in constructing sensitive torsion balances and using them to study Einstein's equivalence principle and to search for new fundamental forces. He is also interested in several problems in high energy astrophysics, dark matter and cosmology, and encourages students join him in this exciting research enterprise. Selected Publications: R. Cowsik, P.N. Bhat, V.R. Chitnis, B.S. Acharya and P.R. Vishwanath (2002) A possible high altitude high energy gamma ray observatory in India, Proc. International Conference on Multi-Colour Universe, TIFA, Mumbai, September 2001, eds. R. K. Manchanda & B. Paul, p. 299, 2002. R. Cowsik, R. Srinivasan & T. P. Prabhu (2002) An Introduction to the Indian Astronomical Observatory, Hanle, Bull. Astr. Soc. India, 30, 105-114. Non-Solar Gamma Rays. Eds. R. Cowsik & R.D.Wills, Pergamon Press, Oxford, NY, 1980 Cosmic Pathways. Ed. R. Cowsik, Tata McGraw Hill Press, 1985 Proc. International Conference on Non-Accelerator Particle Physics, Ed. R. Cowsik, World Scientific Publishing Company, Singapore, 1995
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