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Friedrich Hasenöhrl

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867:... more generally the reason he achieved an incorrect result on both occasions is that he wants to rigorously equate the work performed to kinetic energy, as the work-energy theorem demands. Unfortunately, he does not know how to properly compute the energy. In particular, Hasenöhrl does not conceive of the fact that if the radiators are losing energy, they must be losing mass, which contains an element of irony because it is precisely a mass-energy relation that he is trying to establish. 755:. This case is of historic interest, since it can be treated by electrodynamics alone, even without relativity theory. Then one necessarily comes to ascribe momentum and thus inertial mass to the moving radiation energy. It's interesting that this result was already found by F. Hasenöhrl before the introduction of relativity theory. However, his conclusions were in some points in need of correction. A complete solution of this problem was first given by K. v. Mosengeil. 31: 869:
Let us end by saying that Fritz Hasenöhrl attempted a legitimate thought experiment and tackled it with the tools available at the time. He was working during a transition period and did not create the new theory necessary to allow him to solve the problem correctly and completely. Nevertheless, his
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in 2011 (and Boughn in 2012), who gave a historical account of different solutions to the problem, argued that the above explanation is insufficient. After providing a complete relativistic description and solution of the cavity problem (in the "constant velocity case" and "slow acceleration case"),
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In some additional papers (1907, 1908) Hasenöhrl elaborated further on his 1904-work and concluded that his new results were now in accordance to the theories of Mosengeil and Planck. However, he complained about the fact that Planck (1907) did not mention his earlier 1904-results (like the
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and others argued that this problem is analogous to the so-called 4/3 problem of electromagnetic mass. That is, if Hasenöhrl had included the shell in his calculations in a way consistent with relativity, the pre-factor of 4/3 would have been 1, so yielding
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In 1907 he became Boltzmann's successor at the University of Vienna as the head of the Department of Theoretical Physics. He had a number of illustrious pupils there and had an especially significant impact on
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for every body whose temperature is different from 0° A.. In particular, every body must have an apparent mass determined by the inner radiation, and which is therefore above all dependent on the temperature.
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However, it was shown by Abraham that Hasenöhrl's calculation for the apparent mass was incorrect, so he published another paper in 1905, where he presented Abraham's criticism and corrected his formula to:
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Following this line of thought, Hasenöhrl (1904, 1905) published several papers on the inertia of a cavity containing radiation. This was an entirely classical (non-relativistic) derivation and used
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is the radiation energy. He also concluded that this result is valid for all radiating bodies, i.e. for all bodies whose temperature is > 0K. For this result Hasenöhrl was awarded the
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in 1874. His father was a lawyer and his mother belonged to a prominent aristocratic family. After his elementary education, he studied natural science and mathematics at the
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dependency of apparent mass on temperature). In 1908 Planck wrote that the results of Hasenöhrl's new approach from 1907 were indeed equivalent to those of relativity.
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similar to the famous Einstein's (1905) equation for mass–energy equivalence, that of which the special case of a stationary massive body is widely known as
1128:(1907-1908), Sitzungsberichte der mathematisch-naturwissenschaftlichen Klasse der kaiserlichen Akademie der Wissenschaften, Wien. 116 IIa (9): 1391-1405, 699:
formula given above. Hasenöhrl's results (concerning apparent mass and thermodynamics) by using cavity radiation was further elaborated and criticized by
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In an autobiography, Schrödinger claimed "no other human being had a greater influence on me than Fritz Hasenöhrl, except perhaps my father Rudolph".
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with a thesis titled "Über den Temperaturkoeffizienten der Dielektrizitätskonstante in Flüssigkeiten und die Mosotti-Clausius'sche Formel".
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Since the heat content of every body partly consists of radiating heat, the things that we have demonstrated at a cavity, are true
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broke out in 1914, he volunteered at once into the Austria-Hungarian army. He fought as Oberleutnant against the Italians in
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Married Ella Brückner and had at least one known son, Victor Hasenohrl (? - 1982) who married Elizabeth Sayre (? - 1968)
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energy had been known long before Hasenöhrlt, Einstein was indeed the first to establish the equivalence of
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Albert Einstein's special theory of relativity. Emergence (1905) and early interpretation (1905–1911)
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Afterwards, several authors gave credit to Hasenöhrl for his 1904 achievements on cavity radiation.
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There are different explanations for this result and its deviation from the relativistic formula
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Victor Hasenohrl (? - 1982) who married Elizabeth Sayre (? - 1968) had three adopted children:
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energy-momentum content and understand the deep implications of this principle in
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The equations for electromagnetic mass, like those of Hasenöhrl's (for example,
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Moore, Walter "Schrödinger: Life and Thought" University of Cambridge (1989)
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Sitzungsberichte der Königlich-Preussischen Akademie der Wissenschaften, Berlin
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Translated from the second German edition, G. Bell and sons, London (1950)
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basic conclusion remained valid and for that he should be given credit.
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Fermi, E. (1923). "Sulla massa della radiazione in uno spazio vuoto".
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This was the same relation (as Hasenöhrl noted himself) as for the
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in his work. A broad outline of relativistic thermodynamics and
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at the low temperature laboratory, and there he also befriended
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Zur Theorie der Strahlung in bewegten Körpern. Berichtigung
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Austro-Hungarian military personnel killed in World War I
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Hasenöhrl's papers on cavity radiation and thermodynamics
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who married Victoria ? (?-?) who had two children:
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the speed of light. Subsequently, he used the notation:
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On the Theory of Radiation in Moving Bodies. Correction
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Stephen Boughn (2013). "Fritz Hasenöhrl and E = mc2".
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clarified as early as 1921 that, while the inertia of
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Principle of Relativity"  1226: 995:(1964- ) who lives in Lutherville, Maryland, USA. 1670: 1464:Hasenöhrl and the Equivalence of Mass and Energy 1126:Zur Thermodynamik bewegter Systeme (Fortsetzung) 1365: 1482: 1375:Encyclopädie der Mathematischen Wissenschaften 1451:Another Derivation of Mass-Energy Equivalence 1072:Zur Theorie der Strahlung in bewegten Körpern 221:; 30 November 1874 – 7 October 1915) was an 1344: 1319: 1298: 1081:On the Theory of Radiation in Moving Bodies 1051:On the Theory of Radiation of Moving Bodies 1001:(1966- ) who lives in Boyds, Maryland, USA. 29: 1571: 1498: 1430: 1385: 1302:"On the Dynamics of Moving Systems"  1099:(1905), Annalen der Physik 16, 589-592). 1042:Zur Theorie der Strahlung bewegter Körper 874: 658: 560: 1537: 1074:(1904), Annalen der Physik 15, 344-370. 1172: 1143:On the Thermodynamics of Moving Systems 1671: 1067: 1065: 1063: 1037: 1035: 858:On the other hand, Stephen Boughn and 738:was first pointed out by F. Hasenöhrl. 1462:Stephen Boughn, Tony Rothman (2011): 1390:. Vol. 165. Dover Publications. 1355:, New York: Columbia University Press 1353:Eight lectures on theoretical physics 216: 1233:. Reading: Addison–Wesley. pp.  715:using cavity radiation was given by 335:(1904) used equations equivalent to 1115: 1090: 1060: 1032: 510: 470: 308: 13: 1647:Lebenslauf von Friedrich Hasenöhrl 1608: 1122:Zur Thermodynamik bewegter Systeme 703:(1906/7) who already incorporated 14: 1720: 1640: 1309:. Erster. Halbband (29): 542–570. 1141:English Wikisource translation: 1104:English Wikisource translation: 1079:English Wikisource translation: 1049:English Wikisource translation: 236:Friedrich Hasenöhrl was born in 1709:Physicists from Austria-Hungary 1565: 1531: 1476: 1456: 1443: 1424: 1359: 1338: 1019: 952: 768: 518:{\displaystyle {\mathfrak {B}}} 497:where μ is the apparent mass, E 1652:Career at University of Vienna 1313: 1292: 1251: 1220: 1179: 323:in 1881, many physicists like 16:Austrian physicist (1874–1915) 1: 1167:History of special relativity 501:is the radiation energy, and 1258:Mosengeil, Kurd von (1907). 1199:10.1017/cbo9781139644129.018 753:Radiation in a moving cavity 608:Austrian Academy of Sciences 7: 1486:European Physical Journal H 1187:"Autobiographical Sketches" 1155: 10: 1725: 1517:10.1140/epjh/e2012-30061-5 1227:Miller, Arthur I. (1981). 1132:and 117 IIa (2): 207-215, 312: 1371:"Die Relativitätstheorie" 1328:Physikalische Zeitschrift 973:Frederick Hasenohrl (?- ) 887:(1900), Abraham (1902)), 848:{\displaystyle m=E/c^{2}} 287:for his contributions to 203: 189: 177: 161: 151: 141: 134: 123: 113: 98: 88: 65: 40: 28: 21: 1598:10.1002/andp.19213712005 1556:10.1002/andp.19053231314 1286:10.1002/andp.19073270504 920:{\displaystyle E=mc^{2}} 802:{\displaystyle E=mc^{2}} 1162:Mass–energy equivalence 713:mass-energy equivalence 285:Nobel Prize for Physics 231: 1704:Deaths by hand grenade 1689:Scientists from Vienna 1572:Laue, von, M. (1921). 921: 875:Hasenöhrl and Einstein 872: 849: 803: 766: 749: 686: 620: 588: 519: 487: 405: 265:Heike Kamerlingh Onnes 218:[ˈhaːzn̩øːɐ̯l] 1616:Great Men of Science. 1538:Einstein, A. (1905). 1345:Planck, Max (1915) , 984:Elizabeth Sayre Reich 922: 865: 850: 804: 750: 728: 687: 612: 589: 520: 488: 406: 1388:Theory of Relativity 1320:Planck, Max (1908). 1299:Planck, Max (1907). 1173:Notes and references 895: 818: 777: 734:radiation possesses 709:theory of relativity 697:electromagnetic mass 630: 610:. He wrote in 1904: 532: 505: 436: 416:electromagnetic mass 342: 315:Electromagnetic mass 283:, who later won the 246:University of Vienna 156:University of Vienna 103:University of Vienna 1694:Austrian physicists 1590:1921AnP...371..283L 1561:English translation 1509:2013EPJH...38..261B 1386:Pauli, W. (1981) . 1278:1907AnP...327..867V 993:Daniel Stuart Reich 965:Frederick Hasenohrl 414:for the so-called " 258:Franz-Serafin Exner 210:Friedrich Hasenöhrl 35:Friedrich Hasenöhrl 23:Friedrich Hasenöhrl 1662:2007-09-26 at the 1578:Annalen der Physik 1544:Annalen der Physik 1266:Annalen der Physik 1009:Margaret Hasenohrl 917: 845: 799: 701:Kurd von Mosengeil 682: 584: 515: 483: 401: 1614:Lenard, Philipp, 1433:Rendiconti Lincei 680: 647: 582: 549: 481: 453: 427:pressure of light 425:equation for the 399: 369: 289:quantum mechanics 281:Erwin Schrödinger 207: 206: 198:Erwin Schrödinger 190:Doctoral students 136:Scientific career 83:, Austria-Hungary 1716: 1602: 1601: 1569: 1563: 1559: 1535: 1529: 1528: 1502: 1480: 1474: 1460: 1454: 1447: 1441: 1440: 1428: 1422: 1421: 1415: 1411: 1409: 1401: 1382: 1363: 1357: 1356: 1350: 1342: 1336: 1335: 1325: 1317: 1311: 1310: 1304: 1296: 1290: 1289: 1263: 1255: 1249: 1248: 1224: 1218: 1217: 1216: 1215: 1183: 1150: 1119: 1113: 1094: 1088: 1069: 1058: 1039: 926: 924: 923: 918: 916: 915: 854: 852: 851: 846: 844: 843: 834: 808: 806: 805: 800: 798: 797: 764: 747: 691: 689: 688: 683: 681: 679: 678: 669: 668: 667: 653: 648: 640: 616:mutatis mutandis 593: 591: 590: 585: 583: 581: 580: 571: 570: 569: 555: 550: 542: 524: 522: 521: 516: 514: 513: 492: 490: 489: 484: 482: 480: 479: 474: 473: 466: 465: 456: 454: 446: 410: 408: 407: 402: 400: 398: 397: 388: 387: 375: 370: 362: 357: 356: 309:Cavity radiation 263:He worked under 254:Ludwig Boltzmann 252:(1835–1893) and 220: 215: 179:Doctoral advisor 173: 118:Cavity radiation 93:Austro-Hungarian 72: 51:30 November 1874 50: 48: 33: 19: 18: 1724: 1723: 1719: 1718: 1717: 1715: 1714: 1713: 1669: 1668: 1664:Wayback Machine 1657:Military record 1643: 1611: 1609:Further reading 1606: 1605: 1584:(20): 283–284. 1570: 1566: 1550:(13): 639–641. 1536: 1532: 1481: 1477: 1461: 1457: 1448: 1444: 1429: 1425: 1413: 1412: 1403: 1402: 1398: 1383: 1367:Pauli, Wolfgang 1364: 1360: 1343: 1339: 1318: 1314: 1297: 1293: 1256: 1252: 1245: 1225: 1221: 1213: 1211: 1209: 1185: 1184: 1180: 1175: 1158: 1153: 1120: 1116: 1095: 1091: 1070: 1061: 1040: 1033: 1022: 999:Eric Kent Reich 955: 935:electromagnetic 911: 907: 896: 893: 892: 877: 868: 839: 835: 830: 819: 816: 815: 793: 789: 778: 775: 774: 771: 765: 759: 748: 742: 705:Albert Einstein 674: 670: 663: 659: 654: 652: 639: 631: 628: 627: 604:Haitinger Prize 601: 576: 572: 565: 561: 556: 554: 541: 533: 530: 529: 509: 508: 506: 503: 502: 500: 475: 469: 468: 467: 461: 457: 455: 445: 437: 434: 433: 393: 389: 380: 376: 374: 361: 349: 345: 343: 340: 339: 333:Hendrik Lorentz 317: 311: 299:First World War 242:Austria-Hungary 234: 213: 196: 171: 128:Haitinger Prize 99:Alma mater 84: 74: 70: 61: 59:Austria-Hungary 52: 46: 44: 36: 24: 17: 12: 11: 5: 1722: 1712: 1711: 1706: 1701: 1696: 1691: 1686: 1681: 1667: 1666: 1654: 1649: 1642: 1641:External links 1639: 1638: 1637: 1626: 1610: 1607: 1604: 1603: 1564: 1530: 1493:(2): 261–278. 1475: 1455: 1442: 1423: 1414:|journal= 1396: 1358: 1337: 1334:(23): 828–830. 1312: 1291: 1272:(5): 867–904. 1250: 1243: 1219: 1207: 1177: 1176: 1174: 1171: 1170: 1169: 1164: 1157: 1154: 1152: 1151: 1149: 1148: 1147: 1146: 1114: 1112: 1111: 1110: 1109: 1089: 1087: 1086: 1085: 1084: 1059: 1057: 1056: 1055: 1054: 1030: 1029: 1028: 1026: 1021: 1018: 1017: 1016: 1015: 1014: 1013: 1012: 1006: 1005: 1004: 1003: 1002: 996: 981: 980: 979: 978: 977: 974: 954: 951: 914: 910: 906: 903: 900: 876: 873: 842: 838: 833: 829: 826: 823: 796: 792: 788: 785: 782: 770: 767: 761:Wolfgang Pauli 757: 740: 693: 692: 677: 673: 666: 662: 657: 651: 646: 643: 638: 635: 599: 596: 595: 579: 575: 568: 564: 559: 553: 548: 545: 540: 537: 512: 498: 495: 494: 478: 472: 464: 460: 452: 449: 444: 441: 412: 411: 396: 392: 386: 383: 379: 373: 368: 365: 360: 355: 352: 348: 313:Main article: 310: 307: 233: 230: 205: 204: 201: 200: 191: 187: 186: 184:Franz S. 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Index


Vienna
Austria-Hungary
Vielgereuth
Welschtirol
Austro-Hungarian
University of Vienna
PhD
Cavity radiation
Haitinger Prize
Physicist
University of Vienna
Thesis
Doctoral advisor
Franz S. Exner
Karl Herzfeld
Erwin Schrödinger
[ˈhaːzn̩øːɐ̯l]
Austrian
physicist
Vienna
Austria-Hungary
University of Vienna
Joseph Stefan
Ludwig Boltzmann
Franz-Serafin Exner
Heike Kamerlingh Onnes
Leiden
H. A. Lorentz
Erwin Schrödinger

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