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Marie-No\"elle C\'el\'erier

Identifiers

  • name variant Marie-No\"elle C\'el\'erier 0.60 · backfill

Papers (18)

  1. The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics astro-ph.CO · 2025 · author #288
  2. Redshift and redshift-drift in $\Lambda = 0$ quasi-spherical Szekeres cosmological models and the effect of averaging astro-ph.CO · 2014 · author #2
  3. Redshift-drift as a test for discriminating between decelerating inhomogeneous and accelerating universe models astro-ph.CO · 2013 · author #2
  4. Emergence of complex and spinor wave functions in Scale Relativity. II. Lorentz invariance and bi-spinors physics.gen-ph · 2013 · author #1
  5. Fully Characterizing Axially Symmetric Szekeres Models With Three Data Sets gr-qc · 2012 · author #1
  6. Emergence of complex and spinor wave functions in scale relativity. I. Nature of scale variables physics.gen-ph · 2012 · author #2
  7. Redshift drift in axially symmetric quasi-spherical Szekeres models astro-ph.CO · 2012 · author #2
  8. Effects of inhomogeneities on the expansion of the Universe: a challenge to dark energy? astro-ph.CO · 2012 · author #1
  9. Some clarifications about Lema\^itre-Tolman models of the Universe used to deal with the dark energy problem astro-ph.CO · 2011 · author #1
  10. Inhomogeneous cosmological models: exact solutions and their applications astro-ph.CO · 2011 · author #2
  11. Electromagnetic Klein-Gordon and Dirac equations in scale relativity physics.gen-ph · 2010 · author #1
  12. Szekeres Swiss-Cheese model and supernova observations astro-ph.CO · 2010 · author #2
  13. Motion equations for relativistic particles in an external electromagnetic field in scale relativity physics.gen-ph · 2009 · author #1
  14. A (giant) void is not mandatory to explain away dark energy with a Lemaitre - Tolman model astro-ph.CO · 2009 · author #1
  15. Scaling Regimes as obtained from the DR5 Sloan Digital Sky Survey astro-ph · 2008 · author #2
  16. Is the apparent acceleration of the Universe expansion driven by a dark energy-like component or by inhomogeneities? astro-ph · 2006 · author #1
  17. Quantum-classical transition in Scale Relativity quant-ph · 2006 · author #1
  18. Non-Abelian gauge field theory in scale relativity hep-th · 2006 · author #2

Mentions

  • 1403.5229 #2 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1301.4358 #2 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1301.2186 #1 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1212.3439 #1 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1211.0490 #2 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1206.6026 #2 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1203.2814 #1 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1108.1373 #1 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1102.1449 #2 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1009.2934 #1 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 1005.2584 #2 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 0911.2488 #1 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 0906.0905 #1 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier
  • 0802.0464 #2 · backfill · confidence 0.70 Marie-No\"elle C\'el\'erier

Frequent Coauthors