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Browsing by Author "Sivaram, C"

Browsing by Author "Sivaram, C"

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  • Sivaram, C; Sinha, K. P (American Physical Society, 1977-09)
    Certain similarities and analogies between the properties of black holes and elementary particles are considered in the framework of the strong gravitational field. Properties examined include measurable parameters (mass, ...
  • de Sabbata, V; Sivaram, C (Italian Physical Society, 1989-02)
    We consider the presence of the spin-torsion strong interaction in the proton-proton scattering at several GeV with the aim to see its significance in the anomalous behaviour shown by the scattering cross-section of polarized ...
  • Sivaram, C; Sinha, K. P (Elsevier, 1979-03)
    The concept of short range strong spin-two (f) field (mediated by massive f-mesons) and interacting directly with hadrons was introduced along with the infinite range (g) field in early seventies. In the present review of ...
  • Sivaram, C (Springer, 2010)
    This chapter provides an over view of: (1) Processes in the solar core and corona; (2) The Sun’s place in the galaxy and universe and uniqueness of the Sun for life on earth; (3) The Sun’s role in Olber’s paradox (darkness ...
  • Sinha, K. P; Sivaram, C; Sudarshan, E. C. G (Springer, 1976)
    Some cosmological consequences of the superfluid vacuum state developed previously by the authors are discussed, particularly with regard to the initial stages of the universe. The transition temperature of the hadronic ...
  • Sivaram, C (Deccan Herald, 2011-05-10)
    PHYSICS The first notes and observations on superconductivity marked the beginning of a race between scientists Heike Kamerlingh Onnes and James Dewar, to liquify helium. C Sivaram documents the series of discoveries ...
  • Sivaram, C (Astronomical Society of India, 1984-12)
  • Sivaram, C; Arun, K (Bentham Open, 2011-08)
    There is a lot of current interest in sources of gravitational waves and active ongoing projects to detect such radiation, such as the LIGO project. These are long wavelength, low frequency gravitational waves. LISA would ...
  • Sivaram, C; Arun, K (Bentham Open, 2011-08)
    Thermal gravitational waves can be generated in various sources such as, in the cores of stars, white dwarfs and neutron stars due to the fermion collisions in the dense degenerate Fermi gas [1-3]. Such high frequency ...
  • Sivaram, C (Astronomical Society of India, 1997)
    Superstring theories for which experimental evidence is meagre are considered a most promising approach to understand the quantum nature of gravity and its unification with other fundamental interactions. The geometric ...
  • Sivaram, C (Deccan Herald, 2007-09-25)
  • Sivaram, C (Deccan Herald, 2009-12-22)
  • Sivaram, C (Deccan Herald, 2009-09-22)
  • de Sabbata, V; Sivaram, C; Garcia de Andrade, L (Springer, 1993-09)
    We study electrodynamics in Einstein-Cartan space-time, that is, in space-time with torsion, and show an analogy with the Chern-Simons gauge-invariant massive electrodynamics. In our case, however, there is no arbitrary ...
  • Sivaram, C; De Sabbata, V (Springer, 1991-02)
    The effects of torsion in the early universe on the subsequent evolution are investigated theoretically. The focus is on the simple Einstein-Cartan generalization of conventional big-bang cosmology studied by de Sabbata ...
  • Sivaram, C; de Andrade, L. C. G (Springer, 1994-06)
    A recent model based on massive electrodynamics in spaces with torsion gave rise to London type equations with Meissner-like effects and photon mass. This effective photon mass can be related to a time-varying torsion ...
  • de Sabbata, V; Sivaram, C (Springer, 1990-03)
    A promising possibility which has yet to be considered with a view to furthering understanding of the cosmological constant problem is the use of torsion in a framework such as that of Einstein-Cartan theory: as would be ...
  • de Sabbata, V; Sivaram, C (John Wiley & Sons, Inc., 1990-06)
  • de Sabbata, V; Wang, D. X; Sivaram, C (1990)
  • de Sabbata, V; Sivaram, C (1989)
    The authors consider the effects of torsion on the emission of neutrinos in a hot dense neutron medium and they explore the consequences for the case of SN 1987A neutrinos.

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