Thomas Buchert

Prof. Dr. Thomas Buchert

Centre de Recherche Astrophysique de Lyon, Université de Lyon and École Normale Supérieure de Lyon, F-69364 Lyon CEDEX, France
orcid

Research Focus & Metrics

Academic Career Length

40Years (1987-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

View All Publications
1 January 2000 in General Relativity and Gravitation
Verified
Journal Article
Closed access
PDF file
Thomas BuchertThomas Buchert
Thomas Buchert

11 December 2007 in General Relativity and Gravitation
Verified
Journal Article
Closed access
PDF file
Thomas BuchertThomas Buchert
Thomas Buchert

1 August 2001 in General Relativity and Gravitation
Verified
Journal Article
Closed access
PDF file
Thomas BuchertThomas Buchert
Thomas Buchert

23 November 2012 in Annual Review of Nuclear and Particle Science
Verified
Journal Article
Closed access
Thomas BuchertThomas Buchert
Thomas Buchert
SRSyksy Räsänen
Syksy Räsänen
We review the effect of the formation of nonlinear structures on the expansion rate, spatial curvature, and light propagation in the universe, focusing on the possibility that this effect could explain cosmological observations without requiring the introduction of dark energy or modified gravity. We concentrate on explaining the relevant physics and highlighting open questions.

13 October 2015 in Classical and Quantum Gravity
Verified
Journal Article
Open access
Thomas BuchertThomas Buchert
Thomas Buchert
MCM Carfora
M Carfora
GEG F R Ellis
G F R Ellis
EKE W Kolb
E W Kolb
MMM A H MacCallum
M A H MacCallum
DWDavid L Wiltshire
David L Wiltshire
No. In a number of papers, Green and Wald argue that the standard FLRW model approximates our Universe extremely well on all scales, except close to strong-field astrophysical objects. In particular, they argue that the effect of inhomogeneities on average properties of the Universe (backreaction) is irrelevant. We show that this latter claim is not valid. Specifically, we demonstrate, referring to their recent review paper, that (i) their two-dimensional example used to illustrate the fitting problem differs from the actual problem in important respects, and it assumes what is to be proven; (ii) the proof of the trace-free property of backreaction is unphysical and the theorem about it fails to be a mathematically general statement; (iii) the scheme that underlies the trace-free theorem does not involve averaging and therefore does not capture crucial non-local effects; (iv) their arguments are to a large extent coordinate-dependent, and (v) many of their criticisms of backreaction frameworks do not apply to the published definitions of these frameworks. It is therefore incorrect to infer that Green and Wald have proven a general result that addresses the essential physical questions of backreaction in cosmology.

10 June 1997 in The Astrophysical Journal
Verified
Journal Article
Open access
PDF file
JSJens Schmalzing
Jens Schmalzing
Thomas BuchertThomas Buchert
Thomas Buchert
The genus statistics of isodensity contours has become a well-established tool in cosmology. In this Letter we place the genus in the wider framework of a complete family of morphological descriptors. These are known as the Minkowski functionals, and we here apply them for the first time to isodensity contours of a continuous random field. By taking two equivalent approaches, one through differential geometry, the other through integral geometry, we derive two complementary formulae suitable for numerically calculating the Minkowski functionals. As an example we apply them to simulated Gaussian random fields and compare the outcome to the analytically known results, demonstrating that both are indeed well suited for numerical evaluation. The code used for calculating all Minkowski functionals is available from the authors.Comment: 8 pages plus 1 figure; uses aaspp4.sty and flushrt.sty. Matches version accepted for publication in Ap. J. Let