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papers

Publications (39)

gr-qc1999

Solving the horizon problem with a Delayed Big-Bang singularity

Marie-NoÃ«lle CÃ©lÃ©rier

gr-qc2026

Precision cosmology with exact inhomogeneous solutions of General Relativity: the Szekeres models

Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph.CO2026

A ready-to-fit inhomogeneous cosmological model: The axially symmetric Szekeres spacetime

Marie-NoÃ«lle CÃ©lÃ©rier

hep-th2006

Non-Abelian gauge field theory in scale relativity

Laurent Nottale, Marie-NoÃ«lle CÃ©lÃ©rier, Thierry Lehner

quant-ph2007

Derivation of the postulates of quantum mechanics from the first principles of scale relativity

Laurent Nottale, Marie-NoÃ«lle CÃ©lÃ©rier

gr-qc2000

Models of Universe with a Delayed Big-Bang singularity. III. Solving the horizon problem for an off-center observer

Marie-NoÃ«lle CÃ©lÃ©rier

physics.gen-ph2009

Inhomogeneities in the Universe with exact solutions of General Relativity

Marie-NoÃ«lle CÃ©lÃ©rier

physics.gen-ph2009

Study of chaotic motion in fluid mechanics with the scale relativity methods

Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph.CO2011

Inhomogeneous cosmological models: exact solutions and their applications

Krzysztof Bolejko, Marie-NoÃ«lle CÃ©lÃ©rier, Andrzej KrasiÅski

astro-ph2000

SNIa data to probe the Cosmological Principle

Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph2008

Scaling Regimes as obtained from the DR5 Sloan Digital Sky Survey

Reuben Thieberger, Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph2007

Do we really see a cosmological constant in the supernovae data ?

Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph.CO2010

A (giant) void is not mandatory to explain away dark energy with a Lemaitre - Tolman model

Marie-NoÃ«lle CÃ©lÃ©rier, Krzysztof Bolejko, Andrzej KrasiÅski

gr-qc2023

Fully integrated interior solutions of GR for stationary rigidly rotating cylindrical perfect fluids

Marie-NoÃ«lle CÃ©lÃ©rier

physics.flu-dyn2009

Chaotic motion in classical fluids with scale relativistic methods

Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph2007

Inhomogeneities in the Universe and the Fitting Problem

Marie-NoÃ«lle CÃ©lÃ©rier

physics.gen-ph2009

Motion equations for relativistic particles in an external electromagnetic field in scale relativity

Marie-NoÃ«lle CÃ©lÃ©rier, Laurent Nottale

astro-ph2000

Relativistic corrections to fractal analyses of the galaxy distribution

Marie-NoÃ«lle CÃ©lÃ©rier, Reuben Thieberger

physics.gen-ph2013

Emergence of complex and spinor wave functions in scale relativity. I. Nature of scale variables

Laurent Nottale, Marie-NoÃ«lle CÃ©lÃ©rier

gr-qc2021

New classes of exact interior nonvacuum solutions to the GR field equations for spacetimes sourced by a rigidly rotating stationary cylindrical anisotropic fluid

Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph.CO2025

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

gr-qc2023

Study of stationary rigidly rotating anisotropic cylindrical fluids with new exact interior solutions of GR. 3. Azimuthal pressure

Marie-NoÃ«lle CÃ©lÃ©rier

gr-qc2020

Stationary cylindrical anisotropic fluid and new purely magnetic GR solutions

Marie-NoÃ«lle CÃ©lÃ©rier, Nilton O. Santos

gr-qc2023

Interior spacetimes sourced by stationary differentially rotating irrotational cylindrical fluids. Perfect fluids

Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph2006

Is the apparent acceleration of the Universe expansion driven by a dark energy-like component or by inhomogeneities?

Marie-NoÃ«lle CÃ©lÃ©rier

astro-ph.CO2012

Redshift drift in axially symmetric quasi-spherical Szekeres models

Priti Mishra, Marie-NoÃ«lle CÃ©lÃ©rier, Tejinder P. Singh

physics.gen-ph2010

Electromagnetic Klein-Gordon and Dirac equations in scale relativity

gr-qc2012

Fully Characterizing Axially Symmetric Szekeres Models With Three Data Sets

astro-ph.CO2014

Redshift and redshift-drift in $Î= 0$ quasi-spherical Szekeres cosmological models and the effect of averaging

astro-ph.CO2012

Some clarifications about LemaÃ®tre-Tolman models of the Universe used to deal with the dark energy problem

astro-ph.CO2011

Szekeres Swiss-Cheese model and supernova observations

physics.gen-ph2014

Emergence of complex and spinor wave functions in Scale Relativity. II. Lorentz invariance and bi-spinors

astro-ph.CO2012

Effects of inhomogeneities on the expansion of the Universe: a challenge to dark energy?

gr-qc2024

Interior spacetimes sourced by stationary differentially rotating irrotational cylindrical fluids: anisotropic pressure

quant-ph2006

Quantum-classical transition in Scale Relativity

astro-ph2000

Supernovae data: Cosmological Constant or ruling out the Cosmological Principle ?

astro-ph2007

The Accelerated Expansion of the Universe Challenged by an Effect of the Inhomogeneities. A Review

gr-qc2025

Gravitational collapse of anisotropic cylindrical shearfree fluids with new exact interior solutions of GR

astro-ph.CO2013

Publications (39)

Solving the horizon problem with a Delayed Big-Bang singularity

Precision cosmology with exact inhomogeneous solutions of General Relativity: the Szekeres models

A ready-to-fit inhomogeneous cosmological model: The axially symmetric Szekeres spacetime

Non-Abelian gauge field theory in scale relativity

Derivation of the postulates of quantum mechanics from the first principles of scale relativity

Models of Universe with a Delayed Big-Bang singularity. III. Solving the horizon problem for an off-center observer

Inhomogeneities in the Universe with exact solutions of General Relativity

Study of chaotic motion in fluid mechanics with the scale relativity methods

Inhomogeneous cosmological models: exact solutions and their applications

SNIa data to probe the Cosmological Principle

Scaling Regimes as obtained from the DR5 Sloan Digital Sky Survey

Do we really see a cosmological constant in the supernovae data ?

A (giant) void is not mandatory to explain away dark energy with a Lemaitre - Tolman model

Fully integrated interior solutions of GR for stationary rigidly rotating cylindrical perfect fluids

Chaotic motion in classical fluids with scale relativistic methods

Inhomogeneities in the Universe and the Fitting Problem

Motion equations for relativistic particles in an external electromagnetic field in scale relativity

Relativistic corrections to fractal analyses of the galaxy distribution

Emergence of complex and spinor wave functions in scale relativity. I. Nature of scale variables

New classes of exact interior nonvacuum solutions to the GR field equations for spacetimes sourced by a rigidly rotating stationary cylindrical anisotropic fluid

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Study of stationary rigidly rotating anisotropic cylindrical fluids with new exact interior solutions of GR. 3. Azimuthal pressure

Stationary cylindrical anisotropic fluid and new purely magnetic GR solutions

Interior spacetimes sourced by stationary differentially rotating irrotational cylindrical fluids. Perfect fluids

Is the apparent acceleration of the Universe expansion driven by a dark energy-like component or by inhomogeneities?

Redshift drift in axially symmetric quasi-spherical Szekeres models

Electromagnetic Klein-Gordon and Dirac equations in scale relativity

Fully Characterizing Axially Symmetric Szekeres Models With Three Data Sets

Redshift and redshift-drift in $Î= 0$ quasi-spherical Szekeres cosmological models and the effect of averaging

Some clarifications about LemaÃ®tre-Tolman models of the Universe used to deal with the dark energy problem

Szekeres Swiss-Cheese model and supernova observations

Emergence of complex and spinor wave functions in Scale Relativity. II. Lorentz invariance and bi-spinors

Effects of inhomogeneities on the expansion of the Universe: a challenge to dark energy?

Interior spacetimes sourced by stationary differentially rotating irrotational cylindrical fluids: anisotropic pressure

Quantum-classical transition in Scale Relativity

Supernovae data: Cosmological Constant or ruling out the Cosmological Principle ?

The Accelerated Expansion of the Universe Challenged by an Effect of the Inhomogeneities. A Review

Gravitational collapse of anisotropic cylindrical shearfree fluids with new exact interior solutions of GR

Redshift-drift as a test for discriminating between decelerating inhomogeneous and accelerating universe models

Redshift and redshift-drift in $Î= 0$ quasi-spherical Szekeres cosmological models and the effect of averaging