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Neutronium

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for a long time. Several applications of the dineutron in nuclear reactions can be found in review papers. Its existence has been proven to be relevant for nuclear structure of exotic nuclei. A system made up of only two neutrons is not bound, though the attraction between them is very nearly enough
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The term is not used in the scientific literature either for a condensed form of matter, or as an element, and theoretical analysis expects no bound forms of neutrons without protons. If neutronium were considered to be an element, then these neutron clusters could be considered to be the
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Dineutron: The dineutron, containing two neutrons, is not a stable bound particle, but had been proposed as an extremely short-lived resonance state produced by nuclear reactions involving
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Neutronium is used in popular physics literature to refer to the material present in the cores of neutron stars (stars which are too massive to be supported by
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Hagino, K.; Sagawa, H.; Nakamura, T.; Shimoura, S. (2009). "Two-particle correlations in continuum dipole transitions in Borromean nuclei".
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Pentaneutron: Calculations indicate that the hypothetical pentaneutron state, consisting of a cluster of five neutrons, would not be bound.
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Li, J. G.; Michel, N.; Hu, B. S.; Zuo, W.; Xu, F. R. (2019). "Ab initio no-core Gamow shell-model calculations of multineutron systems".
460: 202:. The resonance was unambiguously observed in 2012 in the decay of beryllium-16. It has been suggested to have a transitory existence in 341: 2717: 248:: A tetraneutron is a hypothetical particle consisting of four bound neutrons. Reports of its existence have not been replicated. 46:, and from the last half of the 20th century onward it has been also used to refer to extremely dense substances resembling the 2502: 911:
MacDonald, J.; Mullan, D. J. (2009). "Big Bang Nucleosynthesis: The Strong Nuclear Force meets the Weak Anthropic Principle".
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and which collapse into a denser phase of matter). In scientific literature the term "neutron-degenerate matter" or simply
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Trineutron: A trineutron state consisting of three bound neutrons has not been detected, and is not expected to be bound.
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Stewart, P. J. (2007). "A century on from Dmitrii Mendeleev: Tables and spirals, noble gases and Nobel prizes".
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Emerson, Edgar I. (1944). "A chart based on atomic numbers showing the electronic structure of the elements".
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The term "neutronium" was coined in 1926 by Andreas von Antropoff for a conjectured form of matter made up of
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Bertulani, C. A.; Zelevinsky, V. (2003). "Is the tetraneutron a bound dineutron-dineutron molecule?".
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two units greater. The dineutron hypothesis had been used in nuclear reactions with
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von Antropoff, A. (1926). "Eine neue Form des periodischen Systems der Elementen".
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of that element. However, these reports have not been further substantiated.
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Ballad of the Stars: Stories of Science Fiction, Ultraimagination, and TRIZ
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Emerson, Edgar I. (1944). "A new spiral form of the periodic table".
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Bevelacqua, J. J. (1981). "Particle stability of the pentaneutron".
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Spyrou, A.; Kohley, Z.; Baumann, T.; Bazin, D.; et al. (2012).
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Gandolfi, Stefano; Gezerlis, Alexandros; Carlson, J. (2015-10-19).
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Timeline of white dwarfs, neutron stars, and supernovae
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Bertulani, C. A.; Canto, L. F.; Hussein, M. S. (1993).
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Schirber, M. (2012). "Nuclei Emit Paired-up Neutrons".
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Timofeyuk, N. K. (2003). "Do multineutrons exist?".
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This has some consequences on 284: 282: 103: 2496: 1193: 1024: 750: 487:Annual Review of Nuclear and Particle Science 364: 355: 288: 30:) is a hypothetical substance made purely of 662: 319: 317: 395: 279: 128:zero at the head of his new version of the 2503: 2489: 1200: 1186: 1144: 323: 1085: 1038: 985: 926: 871: 727: 623: 607: 498: 483:"Neutron Matter from Low to High Density" 314: 175:of approximately 10 minutes), becoming a 71: 2300: 572: 537: 401: 3065: 2354: 2183: 1888: 438: 2484: 2408: 2372: 2363: 2273: 2255: 2246: 1181: 2977: 2417: 2345: 2318: 2291: 1951: 1933: 1906: 1737: 1728: 289:Inglis-Arkell, Esther (2012-04-14). 2426: 2399: 2390: 2237: 2219: 2210: 2201: 1987: 1897: 1870: 1818: 1764: 1746: 1710: 1690: 1629: 1566: 1467: 1449: 1438: 1357: 751:Bertulani, C. A.; Baur, G. (1986). 442:Encyclopedia of Space and Astronomy 61: 50:theorized to exist in the cores of 34:. The word was coined by scientist 13: 2381: 2282: 2165: 2147: 2122: 2113: 2086: 2059: 2014: 1996: 1924: 1915: 1809: 1681: 1647: 1557: 1539: 1530: 1510: 1485: 1207: 517:10.1146/annurev-nucl-102014-021957 237:abundance of the chemical elements 14: 3099: 2336: 2327: 2309: 2264: 2174: 2104: 2077: 2050: 2032: 2023: 2005: 1978: 1960: 1942: 1852: 1782: 1755: 1719: 1665: 1656: 1638: 1620: 1548: 1519: 1458: 1404: 1386: 1348: 1321: 368:Zeitschrift fĂĽr Angewandte Chemie 3050: 3038: 3026: 3014: 3002: 2976: 2967: 2966: 2718:Tolman–Oppenheimer–Volkoff limit 2510: 2228: 2192: 2156: 2041: 1969: 1879: 1861: 1791: 1773: 1701: 1602: 1593: 1584: 1429: 1332: 159:: An isolated neutron undergoes 58:neutronium" will refer to this. 2901:Fermi Gamma-ray Space Telescope 2131: 1836: 1827: 1494: 1476: 1395: 1377: 1138: 1118: 1063: 1018: 959: 904: 849: 744: 693: 656: 463:from the original on 2019-12-15 344:from the original on 2022-04-12 303:from the original on 2014-11-12 2095: 2068: 1611: 1575: 1413: 1368: 729:10.1103/PhysRevLett.108.102501 601: 566: 531: 474: 432: 324:Zhuravleva, Valentina (2005). 1: 2927:X-ray pulsar-based navigation 2906:Compton Gamma Ray Observatory 1800: 575:Journal of Chemical Education 540:Journal of Chemical Education 273: 1169:10.1016/0370-2693(81)91033-9 836:10.1016/0370-1573(93)90128-Z 782:10.1016/0375-9474(88)90467-8 222:as the target nucleus but a 94:electron degeneracy pressure 7: 2896:Rossi X-ray Timing Explorer 2739:Gamma-ray burst progenitors 1104:10.1088/0954-3899/29/10/309 1057:10.1103/PhysRevC.100.054313 255: 104:Hypothetical multi-neutrons 100:is used for this material. 10: 3104: 2952:Most massive neutron stars 2693:Quasi-periodic oscillation 1699: 1528: 1447: 1366: 1330: 1232: 1004:10.1103/PhysRevD.70.043512 945:10.1103/PhysRevD.80.043507 890:10.1103/PhysRevC.80.031301 642:10.1088/0954-3899/29/2/102 65: 2962: 2919: 2911:Chandra X-ray Observatory 2886: 2860: 2731: 2633: 2575: 2539: 2518: 2442: 2142: 1847: 1676: 1505: 1424: 1343: 1316: 1309: 1304: 1299: 1294: 1289: 1284: 1279: 1274: 1269: 1264: 1259: 1254: 1249: 1244: 1239: 1234: 1227: 1222: 1215: 418:10.1007/s10698-007-9038-x 120:, which he placed as the 82:neutron-degenerate matter 48:neutron-degenerate matter 38:in 1926 (before the 1932 3073:Concepts in astrophysics 2678:Neutron-star oscillation 2567:Rotating radio transient 405:Foundations of Chemistry 389:10.1002/ange.19260392303 40:discovery of the neutron 707:Physical Review Letters 2932:Tempo software program 439:Angelo, J. A. (2006). 89: 2947:List of neutron stars 2942:The Magnificent Seven 75: 36:Andreas von Antropoff 2847:Thorne–Żytkow object 1073:Journal of Physics G 687:10.1103/Physics.5.30 611:Journal of Physics G 167:of approximately 15 3088:Fictional materials 2798:Neutron star merger 2658:Chandrasekhar limit 2625:Hulse–Taylor pulsar 2552:Soft gamma repeater 1161:1981PhLB..102...79B 1096:2003JPhG...29.2431B 1049:2019PhRvC.100e4313L 996:2004PhRvD..70d3512K 937:2009PhRvD..80d3507M 882:2009PhRvC..80c1301H 828:1993PhR...226..281B 774:1988NuPhA.480..615B 720:2012PhRvL.108j2501S 679:2012PhyOJ...5...30S 634:2003JPhG...29L...9T 587:1944JChEd..21..254E 552:1944JChEd..21..111E 509:2015ARNPS..65..303G 447:Infobase Publishing 381:1926AngCh..39..722V 2842:Pulsar wind nebula 2820:Stellar black hole 1131:2021-12-13 at the 90: 2990: 2989: 2771:Supernova remnant 2561:Ultra-long period 2478: 2477: 2471: 2470: 2437: 2436: 1148:Physics Letters B 1080:(10): 2431–2437. 1027:Physical Review C 973:Physical Review D 968:McLaughlin, G. C. 914:Physical Review D 859:Physical Review C 761:Nuclear Physics A 595:10.1021/ed021p254 560:10.1021/ed021p111 456:978-0-8160-5330-8 337:978-0-9640740-6-4 204:nuclear reactions 44:changed over time 3095: 3055: 3054: 3043: 3042: 3031: 3030: 3029: 3019: 3018: 3017: 3007: 3006: 2998: 2980: 2979: 2970: 2969: 2744:Asteroseismology 2646:Fast radio burst 2505: 2498: 2491: 2482: 2481: 2447: 2446: 2433: 2431: 2424: 2422: 2415: 2413: 2406: 2404: 2397: 2395: 2388: 2386: 2379: 2377: 2370: 2368: 2361: 2359: 2352: 2350: 2343: 2341: 2334: 2332: 2325: 2323: 2316: 2314: 2307: 2305: 2298: 2296: 2289: 2287: 2280: 2278: 2271: 2269: 2262: 2260: 2253: 2251: 2244: 2242: 2235: 2233: 2226: 2224: 2217: 2215: 2208: 2206: 2199: 2197: 2190: 2188: 2181: 2179: 2172: 2170: 2163: 2161: 2154: 2152: 2138: 2136: 2129: 2127: 2120: 2118: 2111: 2109: 2102: 2100: 2093: 2091: 2084: 2082: 2075: 2073: 2066: 2064: 2057: 2055: 2048: 2046: 2039: 2037: 2030: 2028: 2021: 2019: 2012: 2010: 2003: 2001: 1994: 1992: 1985: 1983: 1976: 1974: 1967: 1965: 1958: 1956: 1949: 1947: 1940: 1938: 1931: 1929: 1922: 1920: 1913: 1911: 1904: 1902: 1895: 1893: 1886: 1884: 1877: 1875: 1868: 1866: 1859: 1857: 1843: 1841: 1834: 1832: 1825: 1823: 1816: 1814: 1807: 1805: 1798: 1796: 1789: 1787: 1780: 1778: 1771: 1769: 1762: 1760: 1753: 1751: 1744: 1742: 1735: 1733: 1726: 1724: 1717: 1715: 1708: 1706: 1697: 1695: 1688: 1686: 1672: 1670: 1663: 1661: 1654: 1652: 1645: 1643: 1636: 1634: 1627: 1625: 1618: 1616: 1609: 1607: 1600: 1598: 1591: 1589: 1582: 1580: 1573: 1571: 1564: 1562: 1555: 1553: 1546: 1544: 1537: 1535: 1526: 1524: 1517: 1515: 1501: 1499: 1492: 1490: 1483: 1481: 1474: 1472: 1465: 1463: 1456: 1454: 1445: 1443: 1436: 1434: 1420: 1418: 1411: 1409: 1402: 1400: 1393: 1391: 1384: 1382: 1375: 1373: 1364: 1362: 1355: 1353: 1339: 1337: 1328: 1326: 1218: 1202: 1195: 1188: 1179: 1178: 1173: 1172: 1142: 1136: 1122: 1116: 1115: 1089: 1067: 1061: 1060: 1042: 1022: 1016: 1015: 989: 987:astro-ph/0312388 966:Kneller, J. P.; 963: 957: 956: 930: 908: 902: 901: 875: 853: 847: 846: 844: 838:. Archived from 811: 802: 793: 792: 790: 784:. Archived from 768:(3–4): 615–628. 757: 748: 742: 741: 731: 697: 691: 690: 660: 654: 653: 627: 605: 599: 598: 570: 564: 563: 535: 529: 528: 502: 478: 472: 471: 469: 468: 436: 430: 429: 399: 393: 392: 362: 353: 352: 350: 349: 321: 312: 311: 309: 308: 286: 218:having the same 122:chemical element 62:In neutron stars 3103: 3102: 3098: 3097: 3096: 3094: 3093: 3092: 3063: 3062: 3061: 3049: 3037: 3027: 3025: 3015: 3013: 3001: 2993: 2991: 2986: 2958: 2915: 2888: 2882: 2856: 2727: 2663:Gamma-ray burst 2653:Bondi accretion 2629: 2571: 2557:Anomalous X-ray 2535: 2514: 2509: 2479: 2474: 2473: 2472: 2438: 2429: 2427: 2420: 2418: 2411: 2409: 2402: 2400: 2393: 2391: 2384: 2382: 2375: 2373: 2366: 2364: 2357: 2355: 2348: 2346: 2339: 2337: 2330: 2328: 2321: 2319: 2312: 2310: 2303: 2301: 2294: 2292: 2285: 2283: 2276: 2274: 2267: 2265: 2258: 2256: 2249: 2247: 2240: 2238: 2231: 2229: 2222: 2220: 2213: 2211: 2204: 2202: 2195: 2193: 2186: 2184: 2177: 2175: 2168: 2166: 2159: 2157: 2150: 2148: 2134: 2132: 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2715: 2710: 2705: 2700: 2695: 2690: 2685: 2680: 2675: 2673:Neutron matter 2670: 2665: 2660: 2655: 2650: 2649: 2648: 2637: 2635: 2631: 2630: 2628: 2627: 2622: 2617: 2612: 2607: 2606: 2605: 2600: 2595: 2585: 2579: 2577: 2576:Binary pulsars 2573: 2572: 2570: 2569: 2564: 2563: 2562: 2559: 2554: 2543: 2541: 2540:Single pulsars 2537: 2536: 2534: 2533: 2528: 2522: 2520: 2516: 2515: 2508: 2507: 2500: 2493: 2485: 2476: 2475: 2469: 2468: 2463: 2458: 2453: 2445: 2443: 2440: 2439: 2435: 2434: 2425: 2416: 2407: 2398: 2389: 2380: 2371: 2362: 2353: 2344: 2335: 2326: 2317: 2308: 2299: 2290: 2281: 2272: 2263: 2254: 2245: 2236: 2227: 2218: 2209: 2200: 2191: 2182: 2173: 2164: 2155: 2146: 2140: 2139: 2130: 2121: 2112: 2103: 2094: 2085: 2076: 2067: 2058: 2049: 2040: 2031: 2022: 2013: 2004: 1995: 1986: 1977: 1968: 1959: 1950: 1941: 1932: 1923: 1914: 1905: 1896: 1887: 1878: 1869: 1860: 1851: 1845: 1844: 1835: 1826: 1817: 1808: 1799: 1790: 1781: 1772: 1763: 1754: 1745: 1736: 1727: 1718: 1709: 1700: 1698: 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Clark 139: 138:Edgar Emerson 135: 134:Charles Janet 131: 127: 126:atomic number 123: 119: 115: 111: 101: 99: 95: 87: 83: 79: 74: 69: 59: 57: 53: 52:neutron stars 49: 45: 41: 37: 33: 29: 25: 21: 2749:Compact star 2723:Urca process 2713:Timing noise 2698:Relativistic 2593:X-ray binary 2588:X-ray pulsar 2512:Neutron star 1152: 1146: 1140: 1120: 1077: 1071: 1065: 1030: 1026: 1020: 977: 971: 961: 918: 912: 906: 863: 857: 851: 840:the original 819: 813: 786:the original 765: 759: 746: 711: 705: 695: 670: 664: 658: 615: 609: 603: 578: 574: 568: 543: 539: 533: 490: 486: 476: 465:. Retrieved 441: 434: 409: 403: 397: 372: 366: 346:. Retrieved 326: 305:. 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Index

neutrons
Andreas von Antropoff
discovery of the neutron
changed over time
neutron-degenerate matter
neutron stars
Neutron star

neutrons
neutron-degenerate matter
quark matter
electron degeneracy pressure
neutron matter
neutrons
protons
electrons
chemical element
atomic number
periodic table
Charles Janet
Edgar Emerson
John D. Clark
isotopes
Neutron
beta decay
mean lifetime
minutes
half-life
proton
nucleus

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