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Particle horizon

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The particle horizon recedes constantly as time passes and the conformal time grows. As such, the observed size of the universe always increases. Since proper distance at a given time is just comoving distance times the scale factor (with
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is not a physically meaningful time (this much time has not yet actually passed); though, as we will see, the particle horizon with which it is associated is a conceptually meaningful distance.
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Margalef-Bentabol, Berta; Margalef-Bentabol, Juan; Cepa, Jordi (February 2013). "Evolution of the cosmological horizons in a universe with countably infinitely many state equations".
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cosmological model. In that context, the universe can be approximated as composed by non-interacting constituents, each one being a perfect fluid with density
66:, it represents the boundary between the observable and the unobservable regions of the universe, so its distance at the present epoch defines the size of the 2406:
Margalef-Bentabol, Berta; Margalef-Bentabol, Juan; Cepa, Jordi (2012-12-21). "Evolution of the cosmological horizons in a concordance universe".
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The concept of a particle horizon can be used to illustrate the famous horizon problem, which is an unresolved issue associated with the
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to travel from where we are located to the furthest observable distance, provided the universe ceased expanding. As such,
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including the curvature state equation. It can be proved that the Hubble function is given by
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which are related as stated before. We have an analogous but slightly different result for
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Any function with a zero subscript denote the function evaluated at the present time
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so well is therefore not explained by the standard explanations about the way the
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Since we observe the CMB to be emitted essentially from our particle horizon (
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normally defined to be equal to proper distance at the present time, so
63: 2217:(2nd ed.). Cambridge: Cambridge University Press. pp. 447–. 641:{\displaystyle a(t)H_{p}(t)=a(t)\int _{0}^{t}{\frac {c\,dt'}{a(t')}}} 427: 2335: 1977:{\displaystyle a_{\text{CMB}}H_{p}(t_{\text{CMB}})=261{\text{ kpc}}} 1726:). Notice that the derivative is made with respect to the FLRW-time 373:{\displaystyle \eta (t_{0})=\eta _{0}=1.48\times 10^{18}{\text{ s}}} 1144:{\displaystyle \Omega ={\frac {\rho }{\rho _{c}}}=\sum \Omega _{i}} 426:. Rather, the conformal time is the amount of time it would take a 2486: 2420: 1393:{\displaystyle H(z)=H_{0}{\sqrt {\sum \Omega _{i0}(1+z)^{n_{i}}}}} 507:
at present), the proper distance to the particle horizon at time
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A primer on the physics of the cosmic microwave background
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Hobson, M. P.; Efstathiou, George; Lasenby, A. N. (2006).
1086:{\displaystyle \Omega _{i}={\frac {\rho _{i}}{\rho _{c}}}} 2170:
proceeds. The most popular resolution to this problem is
1796:(CMB) was emitted, we obtain a particle horizon of about 2244:. Cambridge: Cambridge University Press. pp. 24–. 234:{\displaystyle \eta =\int _{0}^{t}{\frac {dt'}{a(t')}}} 2306:
Publications of the Astronomical Society of Australia
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which corresponds to a proper size at that time of:
1746:, while the functions are evaluated at the redshift 144:. In general, the conformal time at a certain time 1672:{\displaystyle {\frac {dH_{p}}{dt}}=H_{p}(z)H(z)+c} 2366: 2268:General relativity: an introduction for physicists 2206: 2204: 2146: 2107: 2026:(CMB) that are separated by about a fraction of a 2014: 1976: 1908: 1758: 1738: 1714: 1694: 1671: 1584: 1549: 1522: 1499: 1450: 1392: 1298: 1278: 1252: 1222: 1165: 1143: 1085: 1026:{\displaystyle \rho _{c}={\frac {3}{8\pi G}}H^{2}} 1025: 965: 921: 901: 881: 828: 801: 762: 676: 640: 519: 499: 449: 418: 372: 299: 265: 233: 156: 136: 109: 2300:Davis, Tamara M.; Lineweaver, Charles H. (2004). 2241:Cosmological inflation and large-scale structure 50:) is the maximum distance from which light from 2474:Journal of Cosmology and Astroparticle Physics 2408:Journal of Cosmology and Astroparticle Physics 889:, such that they add up to the total density 1702:is the speed of light and can be taken to be 929:. Let us now define the following functions: 419:{\displaystyle 4.35\times 10^{17}{\text{ s}}} 8: 2467: 2465: 2463: 2158:with each other. That the entire CMB is in 2238:Liddle, Andrew R.; Lyth, David H. (2000). 882:{\displaystyle p_{i}=\omega _{i}\rho _{i}} 281:, and we have taken the Big Bang to be at 279:Friedmann–LemaĂ®tre–Robertson–Walker metric 2485: 2419: 2317: 2138: 2126: 2093: 2080: 2065: 2052: 2045: 2037: 2007: 1996: 1991: 1969: 1954: 1941: 1931: 1925: 1897: 1884: 1871: 1853: 1841: 1822: 1809: 1803: 1788:model. Extrapolating back to the time of 1751: 1731: 1707: 1687: 1636: 1612: 1602: 1600: 1565: 1564: 1562: 1541: 1535: 1515: 1483: 1477: 1468: 1466: 1439: 1414: 1408: 1380: 1375: 1350: 1341: 1335: 1314: 1291: 1265: 1244: 1238: 1223:{\displaystyle 1+z={\frac {a_{0}}{a(t)}}} 1198: 1192: 1178: 1158: 1135: 1117: 1108: 1100: 1075: 1065: 1059: 1050: 1044: 1017: 995: 986: 980: 948: 946: 938: 914: 894: 873: 863: 850: 844: 820: 814: 793: 787: 752: 741: 729: 710: 697: 691: 668: 656: 604: 598: 592: 587: 553: 535: 512: 482: 470: 441: 435: 411: 405: 393: 365: 359: 340: 324: 312: 286: 249: 195: 189: 184: 172: 149: 129: 102: 2147:{\displaystyle \theta \sim 1.7^{\circ }} 2022:), our expectation is that parts of the 2200: 966:{\displaystyle H={\frac {\dot {a}}{a}}} 94:, the particle horizon is equal to the 86:Conformal time and the particle horizon 2214:Cosmology: the science of the universe 1451:{\displaystyle n_{i}=3(1+\omega _{i})} 27:Distance measurement used in cosmology 7: 1286:). The last term can be taken to be 1039:-th dimensionless energy density 1347: 1132: 1102: 1047: 380:. Note that the conformal time is 25: 1485: exists if and only if  1095:The dimensionless energy density 774:Evolution of the particle horizon 778:In this section we consider the 2533:Tojero, Rita (March 16, 2006). 1585:{\displaystyle {\dot {a}}>0} 2099: 2086: 2071: 2058: 1960: 1947: 1903: 1890: 1828: 1815: 1660: 1654: 1648: 1642: 1445: 1426: 1372: 1359: 1325: 1319: 1214: 1208: 716: 703: 632: 621: 580: 574: 565: 559: 546: 540: 488: 475: 330: 317: 260: 254: 225: 214: 1: 2504:10.1088/1475-7516/2013/02/015 2438:10.1088/1475-7516/2012/12/035 62:. Much like the concept of a 2543:Royal Observatory, Edinburgh 2365:Giovannini, Massimo (2008). 2211:Harrison, Edward R. (2000). 1403:where the dilution exponent 388:, which is estimated around 2024:cosmic microwave background 1794:cosmic microwave background 54:could have traveled to the 2587: 1777: 1470:The particle horizon  500:{\displaystyle a(t_{0})=1} 117:that has passed since the 2168:expansion of the universe 802:{\displaystyle \rho _{i}} 754: billion light years 450:{\displaystyle \eta _{0}} 1173:given by the formula 975:The critical density 677:{\displaystyle t=t_{0}} 2148: 2109: 2016: 1978: 1910: 1760: 1740: 1716: 1696: 1673: 1586: 1551: 1524: 1501: 1452: 1394: 1300: 1280: 1254: 1224: 1167: 1145: 1087: 1027: 967: 923: 903: 883: 830: 803: 764: 678: 642: 521: 501: 451: 420: 374: 301: 267: 235: 158: 138: 111: 2149: 2110: 2017: 1979: 1911: 1761: 1741: 1717: 1697: 1674: 1587: 1552: 1550:{\displaystyle n_{i}} 1525: 1502: 1453: 1395: 1301: 1281: 1255: 1253:{\displaystyle t_{0}} 1225: 1168: 1146: 1088: 1028: 968: 924: 904: 902:{\displaystyle \rho } 884: 831: 829:{\displaystyle p_{i}} 804: 765: 679: 643: 522: 502: 452: 421: 375: 302: 268: 236: 159: 139: 112: 110:{\displaystyle \eta } 2184:Cosmological horizon 2125: 2036: 1990: 1924: 1802: 1750: 1730: 1706: 1686: 1599: 1561: 1534: 1514: 1465: 1407: 1313: 1290: 1264: 1237: 1177: 1157: 1099: 1043: 979: 937: 913: 893: 843: 813: 786: 690: 655: 534: 511: 469: 434: 392: 311: 285: 266:{\displaystyle a(t)} 248: 171: 148: 128: 101: 48:cosmic light horizon 36:cosmological horizon 18:Cosmic light horizon 2496:2013JCAP...02..015M 2430:2012JCAP...12..035M 2328:2004PASA...21...97D 2189:Observable universe 2162:and approximates a 2160:thermal equilibrium 2154:) should be out of 1279:{\displaystyle z=0} 909:and total pressure 809:, partial pressure 597: 386:age of the universe 300:{\displaystyle t=0} 194: 72:age of the universe 68:observable universe 64:terrestrial horizon 60:age of the universe 2571:Physical cosmology 2144: 2105: 2030:across the sky of 2012: 1974: 1906: 1756: 1736: 1712: 1692: 1669: 1582: 1547: 1520: 1497: 1448: 1390: 1296: 1276: 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Retrieved 2541: 2528: 2477: 2473: 2411: 2407: 2401: 2368: 2360: 2309: 2305: 2295: 2267: 2260: 2240: 2233: 2213: 2119:angular size 2116: 2028:great circle 1985: 1917: 1783: 1681: 1509: 1402: 1232: 1036: 777: 650: 527:is given by 459: 381: 275:scale factor 243: 164:is given by 121:, times the 95: 90:In terms of 89: 47: 39: 35: 31: 29: 2414:(12): 035. 2549:5 November 2480:(2): 015. 2195:References 74:times the 2520:119614479 2512:1475-7516 2487:1302.2186 2454:119704554 2446:1475-7516 2421:1302.1609 2393:191658608 2344:1323-3580 2164:blackbody 2140:∘ 2132:∼ 2129:θ 2009: Gpc 2002:≪ 1998: Mpc 1971: kpc 1873:− 1865:× 1855: Mpc 1839:η 1792:when the 1571:˙ 1437:ω 1348:Ω 1344:∑ 1133:Ω 1129:∑ 1115:ρ 1111:ρ 1103:Ω 1073:ρ 1063:ρ 1048:Ω 1005:π 984:ρ 954:˙ 897:ρ 871:ρ 861:ω 791:ρ 743: Gpc 727:η 585:∫ 439:η 399:× 353:× 338:η 315:η 182:∫ 175:η 105:η 52:particles 2565:Category 2352:13068122 2287:61757089 2178:See also 1786:Big Bang 629:′ 613:′ 222:′ 206:′ 119:Big Bang 56:observer 2492:Bibcode 2476:. 015. 2426:Bibcode 2324:Bibcode 413: s 367: s 277:of the 273:is the 244:where 58:in the 2518:  2510:  2452:  2444:  2391:  2381:  2350:  2342:  2285:  2275:  2248:  2221:  1682:where 1592:) is: 1510:where 428:photon 38:, the 2538:(PDF) 2516:S2CID 2482:arXiv 2450:S2CID 2416:arXiv 2348:S2CID 2314:arXiv 2551:2015 2508:ISSN 2478:2013 2442:ISSN 2412:2012 2389:OCLC 2379:ISBN 2340:ISSN 2283:OCLC 2273:ISBN 2246:ISBN 2219:ISBN 2117:(an 2005:14.4 1577:> 1492:> 1035:The 836:and 780:FLRW 750:46.9 739:14.4 396:4.35 384:the 350:1.48 42:(in 30:The 2500:doi 2434:doi 2377:–. 2332:doi 2136:1.7 2121:of 2067:CMB 1994:284 1967:261 1956:CMB 1933:CMB 1862:8.9 1851:284 1843:CMB 1824:CMB 382:not 2567:: 2540:. 2514:. 2506:. 2498:. 2490:. 2462:^ 2448:. 2440:. 2432:. 2424:. 2410:. 2387:. 2375:70 2346:. 2338:. 2330:. 2322:. 2310:21 2308:. 2304:. 2281:. 2203:^ 2174:. 1869:10 1770:. 407:17 403:10 361:18 357:10 82:. 2553:. 2522:. 2502:: 2494:: 2484:: 2456:. 2436:: 2428:: 2418:: 2395:. 2354:. 2334:: 2326:: 2316:: 2289:. 2254:. 2227:. 2100:) 2095:0 2091:t 2087:( 2082:p 2078:H 2072:) 2063:t 2059:( 2054:p 2050:H 2043:= 2040:f 1964:= 1961:) 1952:t 1948:( 1943:p 1939:H 1929:a 1904:) 1899:0 1895:t 1891:( 1886:p 1882:H 1876:3 1859:= 1848:= 1835:c 1832:= 1829:) 1820:t 1816:( 1811:p 1807:H 1754:z 1734:t 1722:( 1710:1 1690:c 1667:c 1664:+ 1661:) 1658:z 1655:( 1652:H 1649:) 1646:z 1643:( 1638:p 1634:H 1630:= 1624:t 1621:d 1614:p 1610:H 1606:d 1580:0 1568:a 1543:i 1539:n 1518:N 1495:2 1489:N 1479:p 1475:H 1446:) 1441:i 1433:+ 1430:1 1427:( 1424:3 1421:= 1416:i 1412:n 1382:i 1378:n 1373:) 1369:z 1366:+ 1363:1 1360:( 1355:0 1352:i 1337:0 1333:H 1329:= 1326:) 1323:z 1320:( 1317:H 1294:1 1274:0 1271:= 1268:z 1246:0 1242:t 1215:) 1212:t 1209:( 1206:a 1200:0 1196:a 1190:= 1187:z 1184:+ 1181:1 1161:z 1137:i 1126:= 1119:c 1106:= 1077:c 1067:i 1057:= 1052:i 1037:i 1019:2 1015:H 1008:G 1002:8 998:3 993:= 988:c 959:a 951:a 944:= 941:H 917:p 875:i 865:i 857:= 852:i 848:p 822:i 818:p 795:i 758:. 747:= 736:= 731:0 723:c 720:= 717:) 712:0 708:t 704:( 699:p 695:H 670:0 666:t 662:= 659:t 633:) 626:t 622:( 619:a 610:t 606:d 602:c 594:t 589:0 581:) 578:t 575:( 572:a 569:= 566:) 563:t 560:( 555:p 551:H 547:) 544:t 541:( 538:a 515:t 495:1 492:= 489:) 484:0 480:t 476:( 473:a 443:0 347:= 342:0 334:= 331:) 326:0 322:t 318:( 295:0 292:= 289:t 261:) 258:t 255:( 252:a 226:) 219:t 215:( 212:a 203:t 199:d 191:t 186:0 178:= 152:t 132:c 20:)

Index

Cosmic light horizon
Scott Dodelson
particles
observer
age of the universe
terrestrial horizon
observable universe
age of the universe
speed of light
cosmological model
comoving distance
Big Bang
speed of light
scale factor
Friedmann–Lemaître–Robertson–Walker metric
age of the universe
photon
comoving distance
FLRW
state equation
natural units
event horizon
Horizon problem
Big Bang
recombination
cosmic microwave background
cosmic microwave background
great circle
angular size
causal contact

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