pith. machine review for the scientific record. sign in

T. R. Seshadri

Identifiers

  • name variant T. R. Seshadri 0.60 · backfill

Papers (17)

  1. The generation of helical magnetic field in a viable scenario of Inflationary Magnetogenesis astro-ph.CO · 2018 · author #3
  2. Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions astro-ph.CO · 2016 · author #3
  3. Helical cosmological magnetic fields from extra-dimensions astro-ph.CO · 2014 · author #2
  4. Cosmological Magnetogenesis From Extra-dimensional Gauss Bonnet Gravity astro-ph.CO · 2013 · author #3
  5. Primordial Magnetic Field Limits from CMB Trispectrum - Scalar Modes and Planck Constraints astro-ph.CO · 2013 · author #3
  6. Inflation in Higher Dimensional Gauss-Bonnet Cosmology gr-qc · 2013 · author #3
  7. Cosmic Microwave Background Trispectrum and Primordial Magnetic Field Limits astro-ph.CO · 2011 · author #2
  8. Can f(R) gravity mimic dark energy with constant equation of state parameter ? astro-ph.CO · 2011 · author #3
  9. Primordial Magnetic Field Limits from Cosmic Microwave Background Bispectrum of Magnetic Passive Scalar Modes astro-ph.CO · 2010 · author #3
  10. A CCD photometric study of the newly discovered contact binary ASAS 134738+0410.1 astro-ph.SR · 2010 · author #3
  11. A CCD photometric study of the late type contact binary EK Comae Berenices astro-ph.SR · 2010 · author #3
  12. Photometry of the $\delta$ Scuti star HD 40372 astro-ph.SR · 2010 · author #4
  13. Scalar Field Dark Energy Perturbations and their Scale Dependence astro-ph · 2008 · author #3
  14. Some Consequences of Dark Energy Density varying Exponentially with Scale Factor astro-ph · 2005 · author #2
  15. Small-scale CMB polarization anisotropies due to tangled primordial magnetic fields astro-ph · 2003 · author #2
  16. Cosmic Microwave Background Polarization Signals from Tangled Magnetic Fields astro-ph · 2000 · author #1
  17. Self interacting Brans Dicke cosmology and Quintessence gr-qc · 2000 · author #2

Mentions

  • 0801.2017 #3 · backfill · confidence 0.70 T. R. Seshadri

Frequent Coauthors