- Reply to the referee > Although I find this subject matter to be very interesting, I
- REVIEW ARTICLE Inhomogeneous cosmological models: exact solutions
- Geometry and topology of the quasiplane Szekeres model Andrzej Krasinski*
- General Relativity and Gravitation, Vol. 13, No. l, 1981 ORTOCARTAN--ANew Computer Program for
- General Relativity and Gravitation, Vol. 13, No. 11, 1981 Space-Times with Spherically Symmetric
- GeneraIRelativity and Gravitation, Vol. 15, No. 7, 1983 On the Global Geometry of the Stephani Universe1
- ON THE THERMODYNAMICAL INTERPRETATION OF PERFECT FLUID SOLUTIONS OF THE EINSTEIN EQUATIONS WITH NO SYMMETRY
- Rotating dust solutions of Einstein's equations with 3-dimensional symmetry groups. I.
- Rotating dust solutions of Einstein's equations with 3-dimensional symmetry groups. II.
- arXiv:gr-qc/9707021v29Feb2001 ROTATING DUST SOLUTIONS OF EINSTEIN'S EQUATIONS
- Rotating Bianchi type V dust models generalizing the k1 Friedmann model
- Structure formation in the Lemai^tre-Tolman model Andrzej Krasinski*
- More examples of structure formation in the Lemai^tre-Tolman model Andrzej Krasinski*
- Formation of a galaxy with a central black hole in the Lemai^tre-Tolman model Andrzej Krasinski*
- Mon. Not. R. Astron. Soc. 362, 213228 (2005) doi:10.1111/j.1365-2966.2005.09292.x Formation of voids in the Universe within the Lema^itreTolman model
- Alternative methods of describing structure formation in the Lemaitre-Tolman model Charles Hellaby*
- Avoidance of singularities in spherically symmetric charged dust Andrzej Krasinski* and Krzysztof Bolejko
- Can a charged dust ball be sent through the Reissner-Nordstrom wormhole? Andrzej Krasinski* and Krzysztof Bolejko
- Redshift propagation equations in the 0 0 Szekeres models
- Repeatable light paths in the shearfree normal cosmological models Andrzej Krasinski
- Class. Quantum Grav. 11(1994) 1373. Printed in the UK Stationary cylindricallysymmetric vacuumsolutions with A
- INSTITUTE OF PHYSICS PUBLISHING CLASSICAL AND QUANTUM GRAVITY Class. Quantum Grav. 19 (2002) 5273 PII: S0264-9381(02)52771-4
- G en eral Relativity an d G ravitation , Vol. 29, No. 5, 1997 Editor's Note
- G en eral Relativity an d G ravitation , Vol. 29, No. 7, 1997 Editor's Note
- G en eral Relativity an d G ravitation , Vol. 30, No. 4, 1998 Editor's Note
- G en eral Relativity an d G ravitation , Vol. 30, No. 7, 1998 Editor's Note
- G en eral Relativity an d G ravitation , Vol. 30, No. 11, 1998 Editor's Note
- G en eral Relativity an d G ravitation , Vol. 31, No. 6, 1999 Editor's Note
- General Relativity and Gravitation, Vol. 31, No. 12, 1999 Editor's Note
- General Relativity and Gravitation, Vol. 34, No. 1, January 2002 ( c 2002) EDITOR'S NOTE
- Gen Relativ Gravit (2006) 38:13291330 DOI 10.1007/s10714-006-0313-2
- Gen Relativ Gravit (2007) 39:10431045 DOI 10.1007/s10714-006-0308-z
- Gen Relativ Gravit (2008) 40:15571591 DOI 10.1007/s10714-008-0624-6
- Gen Relativ Gravit (2009) 41:203206 DOI 10.1007/s10714-008-0706-5
- This manuscript is on the well-studied problem of how one can fit large scale cosmo-logical data with inhomogeneous (yet still spherically-symmetric) Lemaitre-Tolman (L-T)
- Dear Dr. Celerier, The above manuscript has been reviewed again by two of our referees.
- THIRD REPLY TO THE REFEREE 1. On "gauge dependence"
- Gen Relativ Gravit (2009) 41:16551660 DOI 10.1007/s10714-009-0825-7
- Gen Relativ Gravit (2008) 40:865876 DOI 10.1007/s10714-007-0574-4
- Gen Relativ Gravit (2007) 39:10531054 DOI 10.1007/s10714-006-0356-4
- G en eral Relativity an d G ravitation , Vol. 31, No. 1, 1999 Editor's Note
- We followed the referee's recommendations wherever we found them acceptable. How-ever, the referee is basically wrong in a few points, and in those places we had to object
- Gen Relativ Gravit (2009) 41:24692484 DOI 10.1007/s10714-009-0856-0
- Dear Editor, We are sorry for the delay in our answer -we had to consult the reply to the
- (This is a comment to the first three red segments:) Perhaps the decreasing perturba-tions of homogeneity would have been "huge" in the far past, but we will never know how
- arXiv:gr-qc/9705078v39Feb2001 ROTATING DUST SOLUTIONS OF EINSTEIN'S EQUATIONS
- Most of the referee's comments point out real deficiencies of our paper, and we are grateful to him/her for the improvement the paper will achieve thereby. Here are our
- Gen Relativ Gravit (2009) 41:421432 DOI 10.1007/s10714-008-0721-6
- Structure formation in the Universe by exact methods Andrzej Krasi nski
- Friedmann limits of rotating hypersurfacehomogeneous dust models
- General Relativity and Gravitation, Vol. 31, No. 11, 1999 Editor's Note
- Dear Professor Sprouse, We wish to lodge a formal appeal against the rejection of our paper which was submitted
- G en eral Relativity an d G ravitation , Vol. 30, No. 9, 1998 Editor's Note
- arXiv:gr-qc/0602090v426Feb2007 Avoidance of singularities in spherically symmetric
- General Relativity and Gravitation, Vol. 32, No. 9, 2000 0001-7701/00/0900-193718.00/0 2000 Plenum Publishing Corporation
- Rotating dust solutions of Einstein's equations with three-dimensional symmetry groups.
- G en eral Relativity an d G ravitation , Vol. 29, No. 11, 1997 Editor's Note
- A&A 518, A21 (2010) DOI: 10.1051/0004-6361/200913581
- General Relativity and Gravitation, Vol. 25, No. 2, 1993 The Program ORTOCARTAN for Algebraic
- Downloaded 09 May 2008 to 193.0.83.155. Redistribution subject to AIP license or copyright; see http://jmp.aip.org/jmp/copyright.jsp Downloaded 09 May 2008 to 193.0.83.155. Redistribution subject to AIP license or copyright; see http://jmp.aip.org/jmp/cop
- G en eral Relativity an d G ravitation , Vol. 30, No. 2, 1998 Editor's Note
- General Relativity and Gravitation, Vol. 31, No. 10, 1999 Editor's Note
- General Relativity and Gravitation, Vol. 33, No. 1, 2001 0001-7701/01/0100-0145$18.00/0 2001 Plenum Publishing Corporation
- Dear Dr. Krasinski: The manuscript "Imitating accelerated expansion of the Universe by matter inhomo-
- General Relativity and Gravitation, Vol. 32, No. 9, 2000 0001-7701/00/0900-1933$18.00/0 2000 Plenum Publishing Corporation
- Gen Relativ Gravit (2009) 41:28672871 DOI 10.1007/s10714-009-0887-6
- G en eral Relativity an d G ravitation , Vol. 29, No. 3, 1997 Editor's Note
- Gen Relativ Gravit (2011) 43:331336 DOI 10.1007/s10714-010-1112-3
- Erratum: Avoidance of singularities in spherically symmetric charged dust [Phys. Rev. D 73, 124033 (2006)]
- General Relativity and Gravitation, Vol. 33, No. 12, December 2001 ( c 2002) Editor's Note
- THE SYSTEM ORTOCARTAN USER'S MANUAL
- You cannot get through Szekeres wormholes: Regularity, topology, and causality in quasispherical Szekeres models
- Gen Relativ Gravit (2010) 42:24532475 DOI 10.1007/s10714-010-0993-5
- General Relativity and Gravitation, Vol. 35, No. 3, March 2003 ( C 2003) The Bianchi Classification
- Gen Relativ Gravit (2009) 41:21792189 DOI 10.1007/s10714-009-0868-9
- Formation of Gyrs old black holes in the center of galaxies within the Lema^itreTolman model
- On the thermodynamical interpretation of perfect fluid solutions of the Einstein equations with no symmetry
- Reply to Referee B > (a) clear up the presentation of the treatment of the critical point,
- Physical and geometrical interpretation of the 0 Szekeres models Charles Hellaby*
- General Relativity and Gravitation, Vol. 32, No. 7, 2000 Editor's Note
- General Relativity and Gravitation, Vol. 33, No. 2, 2001 0001-7701/01/0200-0363$19.50/0 2001 Plenum Publishing Corporation
- arXiv:1107.4897v1[gr-qc]25Jul2011 Noname manuscript No.
- Gen Relativ Gravit (2011) 43:22972306 DOI 10.1007/s10714-011-1187-5
- Vol. 42 (2011) ACTA PHYSICA POLONICA B No 11 COSMOLOGICAL MODELS AND
- Gen Relativ Gravit (2012) 44:81105 DOI 10.1007/s10714-011-1260-0
- Gen Relativ Gravit (2012) 44:239251 DOI 10.1007/s10714-011-1274-7
- arXiv:1202.5970v1[gr-qc]27Feb2012 Apparent horizons in the quasi-spherical Szekeres models
