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INFN Padova)

Identifiers

  • name variant INFN Padova) 0.60 · backfill

Papers (19)

  1. A decade of dark matter searches with ground-based Cherenkov telescopes astro-ph.HE · 2014 · author #2
  2. Non-Gaussianity in the Cosmic Microwave Background Anisotropies at Recombination in the Squeezed limit astro-ph.CO · 2011 · author #2
  3. An Estimator for statistical anisotropy from the CMB bispectrum astro-ph.CO · 2011 · author #2
  4. Relativistic effects and primordial non-Gaussianity in the galaxy bias astro-ph.CO · 2010 · author #2
  5. Non-Gaussianity and the Cosmic Microwave Background Anisotropies astro-ph.CO · 2010 · author #2
  6. The Halo Mass Function from Excursion Set Theory with a Non-Gaussian Trispectrum astro-ph.CO · 2009 · author #3
  7. The Halo Mass Function from Excursion Set Theory. III. Non-Gaussian Fluctuations astro-ph.CO · 2009 · author #3
  8. The Halo Mass Function from Excursion Set Theory. I. Gaussian fluctuations with non-markovian dependence on the smoothing scale astro-ph.CO · 2009 · author #3
  9. The Halo Mass Function from Excursion Set Theory. II. The Diffusing Barrier astro-ph.CO · 2009 · author #3
  10. On the non-Gaussianity from Recombination astro-ph · 2008 · author #6
  11. The impact of cosmic neutrinos on the gravitational-wave background astro-ph · 2008 · author #8
  12. Connecting Low Energy Leptonic CP-violation to Leptogenesis hep-ph · 2006 · author #6
  13. Generating the Curvature Perturbation at the End of Inflation in String Theory astro-ph · 2006 · author #3
  14. Second-Order Cosmological Perturbations from Inflation astro-ph · 2002 · author #5
  15. Supersymmetry and Brane Cosmology hep-ph · 2001 · author #2
  16. Adiabatic and Isocurvature Perturbations from Inflation: Power Spectra and Consistency Relations astro-ph · 2001 · author #4
  17. Anomalous Spectral Statistics of the Asymmetric Rotor Model nucl-th · 2001 · author #2
  18. Oscillations During Inflation and the Cosmological Density Perturbations astro-ph · 2001 · author #4
  19. Sum rules for asymptotic form factors in $e^+ e^- -> W^+ W^-$ scattering hep-ph · 1996 · author #3

Mentions

  • 1404.5017 #2 · backfill · confidence 0.70 INFN Padova)
  • 1109.2043 #2 · backfill · confidence 0.70 INFN Padova)
  • 1107.4304 #2 · backfill · confidence 0.70 INFN Padova)
  • 1011.4374 #2 · backfill · confidence 0.70 INFN Padova)
  • 1001.3957 #2 · backfill · confidence 0.70 INFN Padova)
  • 0910.5125 #3 · backfill · confidence 0.70 INFN Padova)
  • 0903.1251 #3 · backfill · confidence 0.70 INFN Padova)
  • 0903.1250 #3 · backfill · confidence 0.70 INFN Padova)
  • 0903.1249 #3 · backfill · confidence 0.70 INFN Padova)
  • 0811.4584 #6 · backfill · confidence 0.70 INFN Padova)
  • 0805.3234 #8 · backfill · confidence 0.70 INFN Padova)

Frequent Coauthors