Category:Horizons - Revision history

Cosmo All at 09:32, 23 April 2014

2014-04-23T09:32:19Z

Igor: /* References */

2013-10-31T08:39:12Z

‎References

Igor: /* References */

2013-10-31T08:36:29Z

‎References

Igor at 20:26, 7 October 2013

2013-10-07T20:26:24Z

Igor at 20:25, 7 October 2013

2013-10-07T20:25:50Z

Igor at 20:25, 7 October 2013

2013-10-07T20:25:30Z

Cosmo All at 07:00, 29 September 2013

2013-09-29T07:00:09Z

Igor at 11:04, 26 September 2013

2013-09-26T11:04:21Z

Cosmo All at 21:35, 25 September 2013

2013-09-25T21:35:52Z

Cosmo All at 12:40, 25 September 2013

2013-09-25T12:40:25Z

← Older revision		Revision as of 09:32, 23 April 2014
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−	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />, and consider first simple, and then composite models, such as $\Lambda$CDM. The fourth section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=Mukhanov />, and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />. The consequent sections focus on more specific topics, such as the various problems regarding the Hubble sphere, inflation and holography.	+	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology - the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />, and consider first simple, and then composite models, such as $\Lambda$CDM. The fourth section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=Mukhanov />, and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />. The consequent sections focus on more specific topics, such as the various problems regarding the Hubble sphere, inflation and holography.

	==References==		==References==

@@ Line 3: / Line 3: @@
 ==References==
 <references>
-<ref name=Harrison>E. Harrison. Cosmology: the science of the Universe. CUP (1981)</ref>
+<ref name=Harrison>E. Harrison. Cosmology: the science of the Universe. CUP (1981) ISBN 978-0-521-66148-5</ref>
 <ref name="Rindler">W. Rindler. Visual horizons in world-models. [http://adsabs.harvard.edu/abs/1956MNRAS.116..662R MNRAS 116 (6), 662--677 (1956) (1981)]</ref>
 <ref name="Ellis">G.F.R. Ellis and T. Rothman. Lost horizons. Am. J. Phys. 61, 883 (1993)</ref>

@@ Line 6: / Line 6: @@
 <ref name="Rindler">W. Rindler. Visual horizons in world-models. [http://adsabs.harvard.edu/abs/1956MNRAS.116..662R MNRAS 116 (6), 662--677 (1956) (1981)]</ref>
 <ref name="Ellis">G.F.R. Ellis and T. Rothman. Lost horizons. Am. J. Phys. 61, 883 (1993)</ref>
-<ref name="Mukhanov">V.F. Mukhanov. Physical foundations of cosmology (CUP, 2005) ISBN~0521563984</ref>
+<ref name="Mukhanov">V.F. Mukhanov. Physical foundations of cosmology (CUP, 2005) ISBN 0521563984</ref>
-<ref name="BrRubin">K.A. Bronnikov and S.G. Rubin. Black Holes, Cosmology and Extra Dimensions. (WSPC, 2012), ISBN~978-9814374200</ref>
+<ref name="BrRubin">K.A. Bronnikov and S.G. Rubin. Black Holes, Cosmology and Extra Dimensions. (WSPC, 2012), ISBN 978-9814374200</ref>
 <!-- <ref name="Melia">F. Melia. The cosmic horizon.  MNRAS 382 (4), 1917--1921 (2007) [http://arxiv.org/abs/0711.4181 arXiv:0711.4181];<br/>F. Melia and M. Abdelqader, The Cosmological Spacetime,  Int. J. Mod. Phys. D 18, 1889 (2009) [http://arxiv.org/abs/0907.5394 arXiv:0907.5394]</ref> -->
 </references>

← Older revision		Revision as of 20:26, 7 October 2013
Line 1:		Line 1:
−	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />, and consider first simple, and then composite models, such as $\Lambda$CDM. The fourth section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=Mukhanov />. and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />. The consequent sections focus on more specific topics, such as the various problems regarding the Hubble sphere, inflation and holography.	+	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />, and consider first simple, and then composite models, such as $\Lambda$CDM. The fourth section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=Mukhanov />, and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />. The consequent sections focus on more specific topics, such as the various problems regarding the Hubble sphere, inflation and holography.

	==References==		==References==

← Older revision		Revision as of 20:25, 7 October 2013
Line 1:		Line 1:
−	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />, and consider first simple, and then composite models, such as $\Lambda$CDM. The fourth section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=~~Muchanov~~ />. and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />. The consequent sections focus on more specific topics, such as the various problems regarding the Hubble sphere, inflation and holography.	+	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />, and consider first simple, and then composite models, such as $\Lambda$CDM. The fourth section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=Mukhanov />. and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />. The consequent sections focus on more specific topics, such as the various problems regarding the Hubble sphere, inflation and holography.

	==References==		==References==

← Older revision		Revision as of 07:00, 29 September 2013
Line 1:		Line 1:
−	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />. The ~~third~~ section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=Muchanov />. ~~The following sections focus on more specific topics, such as the various problems regarding the Hubble sphere<ref name=Melia />, more realistic composite models (including $\Lambda$CDM),~~ and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />.	+	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />, and consider first simple, and then composite models, such as $\Lambda$CDM. The fourth section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=Muchanov />. and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />. The consequent sections focus on more specific topics, such as the various problems regarding the Hubble sphere, inflation and holography.

	==References==		==References==

← Older revision		Revision as of 12:40, 25 September 2013
Line 1:		Line 1:
−	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler ~~\cite{~~Rindler} and G.F.R. Ellis, T. Rothman ~~\cite{~~Ellis}. The third section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov ~~\cite{~~Muchanov}. The following sections focus on more specific topics, such as the various problems regarding the Hubble sphere, more realistic composite models (including $\Lambda$CDM), and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin ~~\cite{~~BrRubin}.	+	In this chapter we assemble the problems that concern one of the most distinctive features of General Relativity and Cosmology --- the horizons. The first part gives an elementary introduction into the concept in the cosmological context, following and borrowing heavily from the most comprehensible text by E. Harrison <ref name=Harrison />. Then we move to more formal exposition of the subject, making use of the seminal works of W. Rindler<ref name=Rindler /> and G.F.R. Ellis, T. Rothman<ref name=Ellis />. The third section elevates the rigor one more step and explores the causal structure of different simple cosmological models in terms of conformal diagrams, following mostly the efficient approach of V. Mukhanov<ref name=Muchanov />. The following sections focus on more specific topics, such as the various problems regarding the Hubble sphere, more realistic composite models (including $\Lambda$CDM), and inflation. The section on black holes relates the general scheme of constructing conformal diagrams for stationary black hole spacetimes, following mostly the excellent textbook of K. Bronnikov and S. Rubin<ref name=BrRubin />.

	==References==		==References==