View Item 

Show simple item record

Fluid sources for Bianchi I and III space‐times
dc.contributor.authorBayin, Selçuk Ş.en_US
dc.contributor.authorKrisch, Jean P.en_US
dc.date.accessioned2010-05-06T22:29:29Z
dc.date.available2010-05-06T22:29:29Z
dc.date.issued1986-01en_US
dc.identifier.citationBayin, Selçuk Ş.; Krisch, J. P. (1986). "Fluid sources for Bianchi I and III space‐times." Journal of Mathematical Physics 27(1): 262-264. <http://hdl.handle.net/2027.42/70647>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/70647
dc.description.abstractFour analytic solutions to the Einstein field equations are presented. The solutions are parametrized to have either Bianchi I or Bianchi III symmetry. The associated fluid parameters are given and some of them are discussed in detail.en_US
dc.format.extent3102 bytes
dc.format.extent254052 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/octet-stream
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleFluid sources for Bianchi I and III space‐timesen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Physics, University of Michigan, Ann Arbor, Michigan 48109en_US
dc.contributor.affiliationotherDepartment of Physics, Canisius College, Buffalo, New York 14208en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/70647/2/JMAPAQ-27-1-262-1.pdf
dc.identifier.doi10.1063/1.527371en_US
dc.identifier.sourceJournal of Mathematical Physicsen_US
dc.identifier.citedreferenceL. Bianchi, Mem. Soc. Ital. Sci. Nat. Mus. Civ. Stor. Nat. Milano 11, 267 (1978).en_US
dc.identifier.citedreferenceJ. M. Stewart and G. F. R. Ellis, J. Math. Phys. 9, 1072 (1968).en_US
dc.identifier.citedreferenceK. C. Jacobs, Astrophys. J. 155, 379 (1969).en_US
dc.identifier.citedreferenceG. F. R. Ellis and M. A. H. MacCallum, Commun. Math. Phys. 12, 108 (1969).en_US
dc.identifier.citedreferenceA. Harvey, Phys. Rev. D 20, 2077 (1979).en_US
dc.identifier.citedreferenceG. Ftaclas and J. M. Cohen, Phys. Rev. D 19, 1051 (1979).en_US
dc.identifier.citedreferenceD. Lorenz, Phys. Lett. A 79, 19 (1980).en_US
dc.identifier.citedreferenceD. Lorenz, Phys. Lett. A 83, 155 (1981).en_US
dc.identifier.citedreferenceD. Lorenz, Gen. Relativ. Gravit. 13, 795 (1981).en_US
dc.identifier.citedreferenceD. Lorenz, Phys. Lett. A 92, 118 (1982).en_US
dc.identifier.citedreferenceM. J. Reboucas, Nuovo. Cimento, B 67, 120 (1982).en_US
dc.identifier.citedreferenceD. Lorenz, Astrophys. Space Sci. 5, 59, 63, 69 (1982).en_US
dc.identifier.citedreferenceN. A. Batakis and D. Tsoubelis, Phys. Rev. D 26, 2611 (1982).en_US
dc.identifier.citedreferenceA. Harvey, Phys. Rev. D 28, 2121 (1983).en_US
dc.identifier.citedreferenceD. Lorenz, J. Phys. A 16, 575 (1983).en_US
dc.identifier.citedreferenceA. J. Accioly, A. N. Vaidya, and M. M. Som, Phys. Rev. D 28, 1853 (1983).en_US
dc.identifier.citedreferenceD. Lorenz, Acta Phys. Pol. B 14, 479 (1983).en_US
dc.identifier.citedreferenceJ. M. Stewart and G. F. R. Ellis, J. Math. Phys. 9, 1072 (1968).en_US
dc.identifier.citedreferenceThis equation for Bianchi I space‐time can also be written in the following convenient form: 1γ1γ2ddt(γ1γ̇2)−12ddt(γ̇1γ1lnγ1γ23)+ddt(γ̇1γ1)[−1+12lnγ1γ23]=0. This is analogous to the Tolman equation given for the relativistic fluid sphere field equation.en_US
dc.identifier.citedreferenceHere Ai,Ci,Ai,Ci, and B are constants of integration.en_US
dc.identifier.citedreferenceE. Kasner, Am. J. Math. 43, 217 (1921).en_US
dc.identifier.citedreferenceK. C. Jacobs, Astrophys. J. 153, 661 (1968).en_US
dc.identifier.citedreferenceW. Gröbner and N. Hofreiter, Integraltafel (Springer, Berlin, 1949), Vol. 1.en_US
dc.identifier.citedreferenceS. Ş. Bayin and J. P. Krisch, unpublished.en_US
dc.identifier.citedreferenceThese are calculated in the comoving, noncoordinated orthonormal system.en_US
dc.owningcollnamePhysics, Department of


Files in this item

Name:
JMAPAQ-27-1-262-1.pdf
Size:
248.0KB
Format:
PDF
View/Open

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.