zbMATH — the first resource for mathematics

Geometry Search for the term Geometry in any field. Queries are case-independent.
Funct* Wildcard queries are specified by * (e.g. functions, functorial, etc.). Otherwise the search is exact.
"Topological group" Phrases (multi-words) should be set in "straight quotation marks".
au: Bourbaki & ti: Algebra Search for author and title. The and-operator & is default and can be omitted.
Chebyshev | Tschebyscheff The or-operator | allows to search for Chebyshev or Tschebyscheff.
"Quasi* map*" py: 1989 The resulting documents have publication year 1989.
so: Eur* J* Mat* Soc* cc: 14 Search for publications in a particular source with a Mathematics Subject Classification code (cc) in 14.
"Partial diff* eq*" ! elliptic The not-operator ! eliminates all results containing the word elliptic.
dt: b & au: Hilbert The document type is set to books; alternatively: j for journal articles, a for book articles.
py: 2000-2015 cc: (94A | 11T) Number ranges are accepted. Terms can be grouped within (parentheses).
la: chinese Find documents in a given language. ISO 639-1 language codes can also be used.

a & b logic and
a | b logic or
!ab logic not
abc* right wildcard
"ab c" phrase
(ab c) parentheses
any anywhere an internal document identifier
au author, editor ai internal author identifier
ti title la language
so source ab review, abstract
py publication year rv reviewer
cc MSC code ut uncontrolled term
dt document type (j: journal article; b: book; a: book article)
Le Châtelier-Braun principle in cosmological physics. (English) Zbl 1162.83375
Summary: Assuming that dark energy may be treated as a fluid with a well-defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark energy and dark matter, it must be such that the latter gains energy from the former and not the other way around.
83F05Relativistic cosmology
83C55Macroscopic interaction of the gravitational field with matter (general relativity)
80A10Classical thermodynamics, including relativistic
[1]Wetterich C.: Nucl. Phys. B 302, 668 (1988) · doi:10.1016/0550-3213(88)90193-9
[2]Coley A., Bylliard P.: Phys. Rev. D 61, 083503 (2000) · doi:10.1103/PhysRevD.61.083503
[3]Amendola L.: Phys. Rev. D 62, 043511 (2000) · doi:10.1103/PhysRevD.62.043511
[4]Tocchini-Valentini D., Amendola L.: Phys. Rev. D 65, 063508 (2002) · doi:10.1103/PhysRevD.65.063508
[5]Farrar G., Peebles P.J.E.: Astrophys. J. 604, 1 (2004) · doi:10.1086/381728
[6]Horvath R.: Phys. Lett. B 648, 374 (2007) · doi:10.1016/j.physletb.2007.03.037
[7]Mainini R., Bonometto S.: J. Cosmology Astropart Phys. 06, 020 (2007) · doi:10.1088/1475-7516/2007/06/020
[8]Zimdahl W., Pavón D.: Class. Quantum Grav. 24, 5461 (2007) · Zbl 1148.83351 · doi:10.1088/0264-9381/24/22/011
[9]Zimdahl W., Pavón D., Chimento L.P.: Phys. Lett. B 521, 133 (2001) · Zbl 1020.83041 · doi:10.1016/S0370-2693(01)01174-1
[10]Chimento L.P., Jakubi A.S., Pavón D., Zimdahl W.: Phys. Rev. D 67, 083513 (2003) · doi:10.1103/PhysRevD.67.083513
[11]del Campo S., Herrera R., Pavón D.: Phys. Rev. D 70, 043540 (2004) · doi:10.1103/PhysRevD.70.043540
[12]Pavón D., Zimdahl W.: Phys. Lett. B 628, 206 (2005) · doi:10.1016/j.physletb.2005.08.134
[13]Olivares G., Atrio-Barandela F., Pavón D.: Phys. Rev. D 71, 063523 (2005) · doi:10.1103/PhysRevD.71.063523
[14]Olivares G., Atrio-Barandela F., Pavón D.: Phys. Rev. D 74, 043521 (2006) · doi:10.1103/PhysRevD.74.043521
[15]Banerjee N., Pavón D.: Phys. Lett. B 647, 477 (2007) · Zbl 1248.83150 · doi:10.1016/j.physletb.2007.02.035
[16]Chimento, L.P., Forte, M., Kremer, G.M.: arxiv:0711.2646 [astro-ph]
[17]Wang B., Gong Y.G., Abdalla E.: Phys. Lett. B 624, 141 (2005) · doi:10.1016/j.physletb.2005.08.008
[18]Wang B., Lin C.Y., Abdalla E.: Phys. Lett. B 637, 357 (2006) · doi:10.1016/j.physletb.2006.04.009
[19]Wang B., Zang J., Lin C.Y., Abdalla E., Micheletti S.: Nucl. Phys. B 778, 69 (2007) · Zbl 05176740 · doi:10.1016/j.nuclphysb.2007.04.037
[20]Wang, B., Lin, C.Y., Pavón, D., Abdalla, E.: Phys. Lett. B 662, 1 (2008)
[21]Abdalla, E., Abramo, L.R., Sodre, L., Wang, B.: arxiv:0710.1198 [astro-ph]
[22]Das S., Corasaniti P.S., Khoury J.: Phys. Rev. D 73, 083509 (2006) · doi:10.1103/PhysRevD.73.083509
[23]Mainini R., Bonometto S.: Phys. Rev. D 74, 043504 (2006) · doi:10.1103/PhysRevD.74.043504
[24]Kremer G.M.: Gen. Relativ. Gravit. 39, 965 (2007) · Zbl 1129.83358 · doi:10.1007/s10714-007-0428-0
[25]Bertolami, O., Gil Pedro, F., Delliou, M.: arxiv:0705.3118 [astro-ph]
[26]Feng, C., Wang, B., Gong, Y.G., Su, R.K.: JCAP 09 (2007) 005, arxiv:0706.4033 [astro-ph]
[27]Bohemer, C.G., Caldera-Cabral, G., Lazkoz, R., Maartens, R.: arxiv:0801.1565 [gr-qc]
[28]de Groot S.R., van Leeuwen W.A., van Weert Ch.G.: Relativistic Kinetic Theory. North Holland, Amsterdam (1980)
[29]Maartens, R.: astro-ph/9609119
[30]Callen H.B.: Equilibrium Thermodynamics. Wiley, NY (1960)
[31]Reif F.: Fundamentals of Statistical and Thermal Physics. Mc-Graw Hill, NY (1965)
[32]Keizer J.: Statistical Thermodynamics of Nonequilibrium Processes. Springer, NY (1987)
[33]Zimdahl W.: Mon. Not. R. Astron. Soc. 288, 665 (1997)
[34]Calvão M.O., Lima J.A.S., Waga I.: Phys. Lett. A 162, 223 (1992) · doi:10.1016/0375-9601(92)90437-Q
[35]Erickson J.K., Caldwell R.R., Steinhardt P.J., Armendariz-Picon C., Mukhanov V.: Phys. Rev. Lett. 88, 121301 (2002) · doi:10.1103/PhysRevLett.88.121301
[36]Chimento L.P., Pavón D.: Phys. Rev. D 73, 063511 (2006) · doi:10.1103/PhysRevD.73.063511