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N. G. Sanchez

Identifiers

  • name variant N. G. Sanchez 0.60 · backfill

Papers (40)

  1. The Dark Matter distribution function and Halo Thermalization from the Eddington equation in Galaxies astro-ph.CO · 2014 · author #2
  2. Equation of state, universal profiles, scaling and macroscopic quantum effects in Warm Dark Matter galaxies astro-ph.CO · 2013 · author #2
  3. Observational rotation curves and density profiles vs. the Thomas-Fermi galaxy structure theory astro-ph.CO · 2013 · author #3
  4. Warm dark matter primordial spectra and the onset of structure formation at redshift z astro-ph.CO · 2013 · author #3
  5. Towards the Chalonge 17th Paris Cosmology Colloquium 2013: highlights and conclusions of the Chalonge 16th Paris Cosmology Colloquium 2012 physics.gen-ph · 2013 · author #3
  6. Dark matter in galaxies: the dark matter particle mass is about 7 keV astro-ph.CO · 2013 · author #2
  7. Quantum WDM fermions and gravitation determine the observed galaxy structures astro-ph.CO · 2013 · author #3
  8. Fermionic warm dark matter produces galaxy cores in the observed scales because of quantum mechanics astro-ph.CO · 2012 · author #3
  9. Towards the Chalonge 16th Paris Cosmology Colloquium 2012: Highlights and Conclusions of the Chalonge 15th Paris Cosmology Colloquium 2011 astro-ph.CO · 2012 · author #3
  10. Cosmological evolution of warm dark matter fluctuations II: Solution from small to large scales and keV sterile neutrinos astro-ph.CO · 2011 · author #2
  11. Cosmological evolution of warm dark matter fluctuations I: Efficient computational framework with Volterra integral equations astro-ph.CO · 2011 · author #2
  12. Warm dark matter in the galaxies:theoretical and observational progresses. Highlights and conclusions of the chalonge meudon workshop 2011 astro-ph.CO · 2011 · author #2
  13. Highlights and Conclusions of the Chalonge 14th Paris Cosmology Colloquium 2010: `The Standard Model of the Universe: Theory and Observations' astro-ph.CO · 2010 · author #3
  14. Highlights and Conclusions of the Chalonge Meudon Workshop Dark Matter in the Universe astro-ph.CO · 2010 · author #2
  15. The mass of the dark matter particle from theory and observations astro-ph.CO · 2010 · author #3
  16. Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters astro-ph.CO · 2010 · author #7
  17. The pre-inflationary and inflationary fast-roll eras and their signatures in the low CMB multipoles astro-ph.CO · 2009 · author #3
  18. Constant surface gravity and density profile of dark matter astro-ph.CO · 2009 · author #2
  19. Higher order terms in the inflaton potential and the lower bound on the tensor to scalar ratio r astro-ph.CO · 2009 · author #3
  20. Model independent analysis of dark matter points to a particle mass at the keV scale astro-ph.CO · 2009 · author #2
  21. The Effective Theory of Inflation in the Standard Model of the Universe and the CMB+LSS data analysis astro-ph.CO · 2009 · author #4
  22. Quantum slow-roll and quantum fast-roll inflationary initial conditions: CMB quadrupole suppression and further effects on the low CMB multipoles astro-ph · 2008 · author #3
  23. The CMB Quadrupole depression produced by early fast-roll inflation: MCMC analysis of WMAP and SDSS data astro-ph · 2008 · author #3
  24. MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio astro-ph · 2007 · author #3
  25. New Inflation vs. Chaotic Inflation, Higher Degree Potentials and the Reconstruction Program in light of WMAP3 astro-ph · 2007 · author #4
  26. CMB quadrupole suppression: I. Initial conditions of inflationary perturbations astro-ph · 2006 · author #3
  27. CMB quadrupole suppression: II. The early fast roll stage astro-ph · 2006 · author #3
  28. Semiclassical (QFT) and Quantum (String) anti - de Sitter Regimes: New Results hep-th · 2006 · author #3
  29. The SL(2,R)WZWN string model as a deformed oscillator and its classical-quantum string regimes hep-th · 2006 · author #2
  30. Single Field Inflation models allowed and ruled out by the three years WMAP data astro-ph · 2006 · author #2
  31. Statistical Mechanics of the Self-Gravitating Gas: Thermodynamic Limit, Unstabilities and Phase Diagrams astro-ph · 2006 · author #2
  32. Clarifying Slow Roll Inflation and the Quantum Corrections to the Observable Power Spectra astro-ph · 2006 · author #3
  33. Semiclassical (Quantum Field Theory) and Quantum (String) de Sitter Regimes: New Results hep-th · 2005 · author #3
  34. Quantum corrections to the inflaton potential and the power spectra from superhorizon modes and trace anomalies astro-ph · 2005 · author #3
  35. Clarifying Inflation Models: Slow-roll as an expansion in 1/N_{efolds} astro-ph · 2005 · author #3
  36. Quantum corrections to slow roll inflation and new scaling of superhorizon fluctuations astro-ph · 2005 · author #3
  37. The Classical and Quantum Inflaton: the Precise Inflationary Potential and Quantum Inflaton Decay after WMAP astro-ph · 2005 · author #3
  38. Clarifying Inflation Models: the Precise Inflationary Potential from Effective Field Theory and the WMAP data astro-ph · 2004 · author #3
  39. Particle decay during inflation: self-decay of inflaton quantum fluctuations during slow roll astro-ph · 2004 · author #3
  40. The quantum inflaton, primordial perturbations and CMB fluctuations astro-ph · 2004 · author #3

Mentions

  • 1401.0726 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 1310.6355 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 1309.2290 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 1308.1109 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 1307.1847 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 1304.0759 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 1301.1864 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 1204.3090 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 1203.3562 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 1111.0300 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 1111.0290 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 1109.3187 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 1009.3494 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 1007.2411 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 1004.1908 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 1003.6108 #7 · backfill · confidence 0.70 N. G. Sanchez
  • 0912.2994 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 0907.0006 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 0906.4102 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 0901.0922 #2 · backfill · confidence 0.70 N. G. Sanchez
  • 0901.0549 #4 · backfill · confidence 0.70 N. G. Sanchez
  • 0809.0623 #3 · backfill · confidence 0.70 N. G. Sanchez
  • 0804.2387 #3 · backfill · confidence 0.70 N. G. Sanchez

Frequent Coauthors