Knowledge (XXG)

Hubble volume

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829: 27: 841: 913: 877: 388:, and the Hubble constant is thought to be decreasing. Thus, sources of light outside the Hubble horizon but inside the cosmological event horizon can eventually reach us. A fairly counter-intuitive result is that photons we observe from the first ~5 billion years of the universe come from regions that are, and always have been, receding from us at superluminal speeds. 901: 853: 889: 376:
principle pure singularities are impossible; also a proportion of their self-interactions are energetic enough to produce escaping particles via quantum tunneling), meeting the criteria of big bang. The justification of this view is that no subluminal Hubble volume will exist and pointwise superluminal expansion (the generalization of the
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theory) will prevail everywhere or at least in a vast region of the universe. In this cyclic cosmology (there are many other cyclic versions) the universe always expands and does not revert to a smaller default size (non-conformal or expandatory conformal, non-Penrosean expandatory cyclic cosmology).
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the Hubble volume still may eventually arrive inside the sphere and be seen by us. Similarly, in an accelerating universe with a decreasing Hubble constant, the Hubble volume expands with time and can overtake light from sources previously receding relative to us. In both of these circumstances, the
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the Hubble sphere will eventually recede outside the sphere and will never be seen by us. If the shrinkage of the Hubble volume does not stop due to some yet unknown phenomenon (one suggestion is the "early phase transition"), the Hubble volume will become nearly a point (due to the uncertainty
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cosmological event horizon lies beyond the Hubble Horizon. In a universe with an increasing Hubble constant, the Hubble horizon will contract, and its boundary overtakes light emitted by nearer galaxies so that light emitted at earlier times by objects
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is not constant in various cosmological models so that the Hubble limit does not, in general, coincide with a cosmological event horizon. For example, in a decelerating
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TM Davis & CH Linewater (2003). "Expanding Confusion: common misconceptions of cosmological horizons and the superluminal expansion of the universe".
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the Hubble sphere expands with time, and its boundary overtakes light emitted by more distant galaxies so that light emitted at earlier times by objects
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N. Carlevaro & G. Montani (2009). "Study of the Quasi-isotropic Solution near the Cosmological Singularity in Presence of Bulk-Viscosity".
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The center of the Hubble volume and observable universe is arbitrary in relation to the overall universe; instead it is centered around its
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For objects at the Hubble limit, the space between us and the object of interest has an average expansion speed of
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For a discussion of why objects that are outside the Earth's Hubble sphere can be seen from Earth, see
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surrounding an observer beyond which objects recede from that observer at a rate greater than the
893: 881: 845: 733: 707: 558: 532: 495: 469: 39: 82:. The Hubble volume is approximately equal to 10 cubic light years (or about 10 cubic meters). 678: 672: 651: 618: 593: 581: 440: 430: 86: 267: 96: 857: 725: 643: 550: 487: 407: 359: 344: 327:. The Hubble time is the reciprocal of the Hubble constant, and is slightly larger than the 300: 759: 647: 331:(13.8 billion years) as it is the age the universe would have had if expansion was linear. 155: 351:(a boundary separating events visible at some time and those that are never visible). See 180: 397: 324: 721: 546: 483: 917: 833: 306: 149: 131: 75: 927: 737: 348: 90: 797: 562: 912: 869: 812: 499: 47: 250:. However, the term is also frequently (but mistakenly) used as a synonym for the 698:
John L Tonry; et al. (2003). "Cosmological Results from High-z Supernovae".
577: 491: 34:. The inner blue ring indicates the approximate size of the Hubble volume. 712: 537: 377: 79: 554: 864: 729: 474: 25: 617:(2nd ed.). Oxford : Oxford University Press. p. 304. 202:
can be applied to any region of space with a volume of order
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radius of a Hubble sphere (known as the Hubble radius or the
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Observations indicate that the expansion of the universe is
752:"Is the universe expanding faster than the speed of light?" 584:. In Barrow, J. D.; Davies, J. D.; Harper, C. L. (eds.). 642:(2nd ed.). Oxford University Press. p. 225. 817: 525:
Publications of the Astronomical Society of Australia
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Science and Ultimate Reality: From Quantum to Cosmos
315: 291: 242: 171: 140: 120: 613:Hawley, John F.; Holcomb, Katherine A. (2005). 254:; the latter is larger than the Hubble volume. 183:. The surface of a Hubble sphere is called the 8: 677:. Cambridge University Press. p. 439. 588:. Cambridge University Press. pp. 459 424: 422: 711: 536: 473: 462:International Journal of Modern Physics D 308: 283: 274: 269: 234: 224: 215: 207: 163: 157: 133: 112: 103: 98: 824: 756:Ask an Astronomer at Cornell University 517: 515: 513: 511: 509: 418: 575:For an example of mistaken usage, see 261:(impersonal or personal "observer"). 7: 648:10.1093/acref/9780199609055.001.0001 299:is 14.4 billion light years in the 343:. So, in a universe with constant 14: 16:Region of the observable universe 911: 899: 887: 875: 863: 851: 839: 827: 335:Hubble limit as an event horizon 671:Edward Robert Harrison (2000). 615:Foundations of modern cosmology 429:Edward Robert Harrison (2003). 934:Physical cosmological concepts 231: 209: 1: 813:The Hubble Volume Simulations 243:{\displaystyle (c/H_{0})^{3}} 70:is a spherical region of the 803:Resources in other libraries 78:due to the expansion of the 30:Visualization of the whole 301:standard cosmological model 950: 437:Cambridge University Press 46:(named for the astronomer 18: 798:Resources in your library 640:A Dictionary of Astronomy 492:10.1142/S0218271808012553 198:More generally, the term 21:Hubble bubble (astronomy) 19:Not to be confused with 292:{\displaystyle c/H_{0}} 121:{\displaystyle c/H_{0}} 317: 293: 244: 173: 142: 122: 35: 674:Masks of the Universe 638:Ridpath, Ian (2012). 432:Masks of the Universe 318: 294: 245: 185:microphysical horizon 174: 172:{\displaystyle H_{0}} 143: 123: 29: 582:"Parallel Universes" 307: 268: 206: 156: 132: 97: 762:on 23 November 2003 722:2003ApJ...594....1T 547:2004PASA...21...97D 484:2008IJMPD..17..881C 329:age of the universe 252:observable universe 72:observable universe 68:sphere of causality 32:observable universe 364:Friedmann universe 355:for more details. 313: 289: 264:The Hubble length 240: 169: 138: 118: 36: 784:Library resources 684:978-0-521-66148-5 624:978-0-19-853096-1 599:978-0-521-83113-0 446:978-0-521-77351-5 316:{\displaystyle c} 141:{\displaystyle c} 60:subluminal sphere 941: 916: 915: 904: 903: 902: 892: 891: 890: 880: 879: 878: 868: 867: 856: 855: 854: 844: 843: 832: 831: 823: 772: 771: 769: 767: 758:. 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Index

Hubble bubble (astronomy)

observable universe
cosmology
Edwin Hubble
observable universe
speed of light
universe
proper
Hubble length
speed of light
Hubble constant
observable universe
origin
standard cosmological model
Hubble time
age of the universe
Hubble parameter
event horizon
Hubble horizon
Hubble parameter
Friedmann universe
Big Bang
accelerating
Hubble's law
Hubble horizon
Particle horizon


Masks of the Universe

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