リケラボ論文検索は、全国の大学リポジトリにある学位論文・教授論文を一括検索できる論文検索サービスです。

リケラボ 全国の大学リポジトリにある学位論文・教授論文を一括検索するならリケラボ論文検索大学・研究所にある論文を検索できる

リケラボ 全国の大学リポジトリにある学位論文・教授論文を一括検索するならリケラボ論文検索大学・研究所にある論文を検索できる

大学・研究所にある論文を検索できる 「Neutrinos and lepton number oscillations in quantum field theory」の論文概要。リケラボ論文検索は、全国の大学リポジトリにある学位論文・教授論文を一括検索できる論文検索サービスです。

コピーが完了しました

URLをコピーしました

論文の公開元へ論文の公開元へ
書き出し

Neutrinos and lepton number oscillations in quantum field theory

Benoit Nicholas James 広島大学

2022.09.20

概要

Neutrino physics has changed significantly since the discovery of flavor oscillations by Super Kamiokande and the Sudbury Neutrino Observatory. Starting with the work of Pontecovo, the theory of neutrino flavor oscillations in quantum mechanics has been established for some time. However, a consensus for the theory of neutrino flavor oscillations in quantum field theory has not been reached and is an active area of research.

We developed a formulation of neutrino flavor oscillations based on lepton family numbers in quantum field theory. We will start with a derivation of lepton family number for neutrinos with Majorana masses. Then, we will derive the lepton family number for neutrinos with Dirac masses. The main result of those derivations are a Majorana expectation value from our original work and a Dirac expectation value that is new for this thesis.

Some important results from of the expectation values are time dependent oscillations, total lepton number violation or conservation, and the recovery of the quantum mechanics formulation in the ultra-relativistic limit. We also compare the Majorana expectation value and the Dirac expectation value, which is a new comparison for this thesis. We compare them in two ways, first by studying the total lepton number and second by comparing the low momentum phenomenology. For total lepton number, we find the Dirac expectation value to conserve total lepton number, whereas the Majorana expectation value violates total lepton number. In the low momentum phenomenology our formulation has three interesting properties, we can distinguish the neutrino mass type, differences from the neutrino mass hierarchy are enhanced, and the Majorana phases can play an important role to the Majorana Expectation value.

Lastly, we prove our formulation is the same in the Schrödinger and Heisenberg pictures. We study a non-trivial relationship between the Fock spaces of the operators, which is not usually considered in high energy physics. That non-trivial relationship leads to a Bogolyubov transformation that connects the operators of the Fock spaces. This is sometimes considered in Thermal field theory and gives an interesting theoretical background to our model.

参考文献

[1] K. Abe et al. [Super-Kamiokande], Phys. Rev. D 94, no.5, 052010 (2016) doi:10.1103/PhysRevD.94.052010 [arXiv:1606.07538 [hep-ex]].

[2] K. Abe et al. [Super-Kamiokande], Phys. Rev. D 97, no.7, 072001 (2018) doi:10.1103/PhysRevD.97.072001 [arXiv:1710.09126 [hep-ex]].

[3] M. Jiang et al. [Super-Kamiokande], PTEP 2019, no.5, 053F01 (2019) doi:10.1093/ptep/ptz015 [arXiv:1901.03230 [hep-ex]].

[4] P. Adamson et al. [NOvA], Phys. Rev. Lett. 116, no.15, 151806 (2016) doi:10.1103/PhysRevLett.116.151806 [arXiv:1601.05022 [hep-ex]].

[5] M. A. Acero et al. [NOvA], Phys. Rev. D 98, 032012 (2018) doi:10.1103/PhysRevD.98.032012 [arXiv:1806.00096 [hep-ex]].

[6] M. A. Acero et al. [NOvA], Phys. Rev. Lett. 123, no.15, 151803 (2019) doi:10.1103/PhysRevLett.123.151803 [arXiv:1906.04907 [hep-ex]].

[7] J. Schneps, AIP Conf. Proc. 1666, no.1, 190002 (2015) doi:10.1063/1.4915603

[8] C. Giunti and C. W. Kim, “Fundamentals of Neutrino Physics and Astrophysics,”

[9] M. Fukugita and T. Yanagida, “Physics of neutrinos and applica- tions to astrophysics,” doi:10.1007/978-3-662-05119-1

[10] J. Chadwick, Verh. Phys. Gesell. 16, 383-391 (1914)

[11] C. D. Ellis and W. A. Wooster, Proc. Roy. Soc. Lond. A 117, no.776, 109-123 (1927) doi:10.1098/rspa.1927.0168

[12] W. Pauli, “Dear radioactive ladies and gentlemen,”

[13] E. Fermi, Ric. Sci. 4, 491-495 (1933)

[14] H. Bethe and R. Peierls, Nature 133, 532 (1934) doi:10.1038/133532a0

[15] B. Pontecorvo, Report PD-205 of the National Research Council of Canada, Division of Atomic Energy, Chalk River, Ontario, Nov. 13, 1946.

[16] C. L. Cowan, F. Reines, F. B. Harrison, H. W. Kruse and A. D. McGuire, Science 124, 103-104 (1956) doi:10.1126/science.124.3212.103

[17] E. Fermi, Z. Phys. 88, 161-177 (1934) doi:10.1007/BF01351864

[18] G. Gamow and E. Teller, Phys. Rev. 51, 289-289 (1937) doi:10.1103/PhysRev.51.289

[19] B. Pontecorvo, Phys. Rev. 72, 246 (1947) doi:10.1103/PhysRev.72.246

[20] C. S. Wu, E. Ambler, R. W. Hayward, D. D. Hoppes and R. P. Hudson, Phys. Rev. 105, 1413-1414 (1957) doi:10.1103/PhysRev.105.1413

[21] E. Ambler, R. W. Hayward, D. D. Hoppes, R. P. Hudson and C. S. Wu, Phys. Rev. 106, 1361-1363 (1957) doi:10.1103/PhysRev.106.1361

[22] R. P. Feynman and M. Gell-Mann, Phys. Rev. 109, 193-198 (1958) doi:10.1103/PhysRev.109.193

[23] E. C. G. Sudarshan and R. e. Marshak, Phys. Rev. 109, 1860-1860 (1958) doi:10.1103/PhysRev.109.1860.2

[24] J. J. Sakurai, Nuovo Cim. 7, 649-660 (1958) doi:10.1007/BF02781569

[25] A. Salam, Nuovo Cim. 5, 299-301 (1957) doi:10.1007/BF02812841

[26] L. D. Landau, Nucl. Phys. 3, 127-131 (1957) doi:10.1016/0029-5582(57)90061-5

[27] T. D. Lee and C. N. Yang, Phys. Rev. 105, 1671-1675 (1957) doi:10.1103/PhysRev.105.1671

[28] G. Puppi, Nuovo Cim. 5, 587-588 (1948) doi:10.1007/BF02780913

[29] O. Klein, Nature 161, 897-899 (1948) doi:10.1038/161897a0

[30] T. D. Lee, M. Rosenbluth and C. N. Yang, Phys. Rev. 75, 905 (1949) doi:10.1103/PhysRev.75.905

[31] J. Tiomno and J. A. Wheeler, Rev. Mod. Phys. 21, 144-152 (1949) doi:10.1103/RevModPhys.21.144

[32] E. J. Konopinski and H. M. Mahmoud, Phys. Rev. 92, 1045-1049 (1953) doi:10.1103/PhysRev.92.1045

[33] G. Danby, J. M. Gaillard, K. A. Goulianos, L. M. Lederman, N. B. Mis- try, M. Schwartz and J. Steinberger, Phys. Rev. Lett. 9, 36-44 (1962) doi:10.1103/PhysRevLett.9.36

[34] B. Pontecorvo, Zh. Eksp. Teor. Fiz. 37, 1751-1757 (1959)

[35] S. L. Glashow, Nucl. Phys. 22, 579-588 (1961) doi:10.1016/0029-5582(61)90469-2

[36] S. Weinberg, Phys. Rev. Lett. 19, 1264-1266 (1967) doi:10.1103/PhysRevLett.19.1264

[37] A. Salam, Conf. Proc. C 680519, 367-377 (1968) doi:10.1142/9789812795915 0034

[38] F. J. Hasert, H. Faissner, W. Krenz, J. Von Krogh, D. Lanske, J. Morfin, K. Schultze, H. Weerts, G. H. Bertrand-Coremans and J. Lemonne, et al. Phys. Lett. B 46, 121-124 (1973) doi:10.1016/0370- 2693(73)90494-2

[39] F. J. Hasert et al. [Gargamelle Neutrino], Phys. Lett. B 46, 138-140 (1973) doi:10.1016/0370-2693(73)90499-1

[40] F. J. Hasert et al. [Gargamelle Neutrino], Nucl. Phys. B 73, 1-22 (1974) doi:10.1016/0550-3213(74)90038-8

[41] S. Schael et al. [ALEPH, DELPHI, L3, OPAL, SLD, LEP Elec-troweak Working Group, SLD Electroweak Group and SLD Heavy Flavour Group], Phys. Rept. 427, 257-454 (2006) doi:10.1016/j.physrep.2005.12.006 [arXiv:hep-ex/0509008 [hep- ex]].

[42] B. T. Cleveland, T. Daily, R. Davis, Jr., J. R. Distel, K. Lande, C. K. Lee, P. S. Wildenhain and J. Ullman, Astrophys. J. 496, 505-526 (1998) doi:10.1086/305343

[43] A. B. McDonald, Rev. Mod. Phys. 88, no.3, 030502 (2016) doi:10.1103/RevModPhys.88.030502

[44] T. Kajita, Rev. Mod. Phys. 88, no.3, 030501 (2016) doi:10.1103/RevModPhys.88.030501

[45] B. Pontecorvo, Sov. Phys. JETP 6, 429 (1957)

[46] B. Pontecorvo, Zh. Eksp. Teor. Fiz. 34, 247 (1957)

[47] B. Pontecorvo, Zh. Eksp. Teor. Fiz. 53, 1717-1725 (1967)

[48] V. N. Gribov and B. Pontecorvo, Phys. Lett. B 28, 493 (1969) doi:10.1016/0370-2693(69)90525-5

[49] Z. Maki, M. Nakagawa and S. Sakata, Prog. Theor. Phys. 28, 870-880 (1962) doi:10.1143/PTP.28.870

[50] Y. Fukuda et al. [Super-Kamiokande], Phys. Rev. Lett. 81, 1562-1567 (1998) doi:10.1103/PhysRevLett.81.1562 [arXiv:hep-ex/9807003 [hep-ex]].

[51] Q. R. Ahmad et al. [SNO], Phys. Rev. Lett. 89, 011301 (2002) doi:10.1103/PhysRevLett.89.011301 [arXiv:nucl-ex/0204008 [nucl- ex]].

[52] L. Wolfenstein, Phys. Rev. D 17, 2369-2374 (1978) doi:10.1103/PhysRevD.17.2369

[53] S. P. Mikheev and A. Y. Smirnov, Nuovo Cim. C 9, 17-26 (1986) doi:10.1007/BF02508049

[54] S. P. Mikheyev and A. Y. Smirnov, Sov. J. Nucl. Phys. 42, 913-917 (1985)

[55] B. Kayser, Phys. Rev. D 24, 110 (1981) doi:10.1103/PhysRevD.24.110

[56] C. Giunti and C. W. Kim, Found. Phys. Lett. 14, no.3, 213-229 (2001) doi:10.1023/A:1012230026160 [arXiv:hep-ph/0011074 [hep-ph]].

[57] S. Eliezer and A. R. Swift, Nucl. Phys. B 105, 45-51 (1976) doi:10.1016/0550-3213(76)90059-6

[58] S. M. Bilenky and B. Pontecorvo, Yad. Fiz. 24, 603-608 (1976)

[59] S. M. Bilenky and B. Pontecorvo, Lett. Nuovo Cim. 17, 569 (1976) doi:10.1007/BF02746567

[60] R. G. Winter, Lett. Nuovo Cim. 30, 101-104 (1981) doi:10.1007/BF02817319

[61] C. Giunti, C. W. Kim and U. W. Lee, Phys. Rev. D 45, 2414-2420 (1992) doi:10.1103/PhysRevD.45.2414

[62] E. Akhmedov, JHEP 07, 070 (2017) doi:10.1007/JHEP07(2017)070 [arXiv:1703.08169 [hep-ph]].

[63] E. K. Akhmedov and A. Y. Smirnov, Phys. Atom. Nucl. 72, 1363-1381 (2009) doi:10.1134/S1063778809080122 [arXiv:0905.1903 [hep-ph]].

[64] E. Akhmedov, “Quantum mechanics aspects and subtleties of neutrino oscillations,” [arXiv:1901.05232 [hep-ph]].

[65] D. Bohm, “Quantum Theory,”

[66] S. Weinberg, “The Quantum theory of fields. Vol. 1: Foundations,”

[67] M. Zralek, Acta Phys. Polon. B 29, 3925-3956 (1998) [arXiv:hep- ph/9810543 [hep-ph]].

[68] M. Beuthe, Phys. Rept. 375, 105-218 (2003) doi:10.1016/S0370-1573(02)00538-0 [arXiv:hep-ph/0109119 [hep-ph]].

[69] C. Giunti, C. W. Kim, J. A. Lee and U. W. Lee, Phys. Rev. D 48, 4310- 4317 (1993) doi:10.1103/PhysRevD.48.4310 [arXiv:hep-ph/9305276 [hep-ph]].

[70] C. Giunti, C. W. Kim and U. W. Lee, Phys. Lett. B 421, 237-244 (1998) doi:10.1016/S0370-2693(98)00014-8 [arXiv:hep-ph/9709494 [hep-ph]].

[71] K. Kiers and N. Weiss, Phys. Rev. D 57, 3091-3105 (1998) doi:10.1103/PhysRevD.57.3091 [arXiv:hep-ph/9710289 [hep-ph]].

[72] C. Y. Cardall, Phys. Rev. D 61, 073006 (2000) doi:10.1103/PhysRevD.61.073006 [arXiv:hep-ph/9909332 [hep- ph]].

[73] M. Beuthe, Phys. Rev. D 66, 013003 (2002) doi:10.1103/PhysRevD.66.013003 [arXiv:hep-ph/0202068 [hep- ph]].

[74] C. Giunti, JHEP 11, 017 (2002) doi:10.1088/1126-6708/2002/11/017 [arXiv:hep-ph/0205014 [hep-ph]].

[75] Y. V. Shtanov, Phys. Rev. D 57, 4418-4428 (1998) doi:10.1103/PhysRevD.57.4418 [arXiv:hep-ph/9706378 [hep- ph]].

[76] Y. Srivastava, A. Widom and E. Sassaroli, Z. Phys. C 66, 601-605 (1995) doi:10.1007/BF01579634

[77] Y. Srivastava, A. Widom and E. Sassaroli, Eur. Phys. J. C 2, 769-774 (1998) doi:10.1007/s100520050181

[78] M. Blasone, A. Capolupo and G. Vitiello, Phys. Rev. D 66, 025033 (2002) doi:10.1103/PhysRevD.66.025033 [arXiv:hep-th/0204184 [hep-th]].

[79] M. Blasone, A. Capolupo, O. Romei and G. Vitiello, Phys. Rev. D63, 125015 (2001) doi:10.1103/PhysRevD.63.125015 [arXiv:hep-ph/0102048 [hep-ph]].

[80] M. Blasone, P. A. Henning and G. Vitiello, Phys. Lett. B 451, 140-145 (1999) doi:10.1016/S0370-2693(99)00155-0 [arXiv:hep-th/9803157 [hep-th]].

[81] M. Blasone, P. Jizba and G. Vitiello, Phys. Lett. B 517, 471-475 (2001) doi:10.1016/S0370-2693(01)00985-6 [arXiv:hep-th/0103087 [hep-th]].

[82] C. R. Ji and Y. Mishchenko, Phys. Rev. D 64, 076004 (2001) doi:10.1103/PhysRevD.64.076004 [arXiv:hep-ph/0105094 [hep- ph]].

[83] C. R. Ji and Y. Mishchenko, Phys. Rev. D 65, 096015 (2002) doi:10.1103/PhysRevD.65.096015 [arXiv:hep-ph/0201188 [hep- ph]].

[84] S. M. Bilenky and C. Giunti, Int. J. Mod. Phys. A 16, 3931-3949 (2001) doi:10.1142/S0217751X01004967 [arXiv:hep-ph/0102320 [hep-ph]].

[85] T. Hahn, [arXiv:physics/0607103 [physics]].

[86] A. S. Adam, N. J. Benoit, Y. Kawamura, Y. Matsuo, T. Morozumi, Y. Shimizu, Y. Tokunaga and N. Toyota, PTEP 2021, 5 (2021) doi:10.1093/ptep/ptab025 [arXiv:2101.07751 [hep-ph]].

[87] M. Born, Z. Phys. 37, no.12, 863-867 (1926) doi:10.1007/BF01397477

[88] I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, T. Schwetz and A. Zhou, JHEP 09, 178 (2020) doi:10.1007/JHEP09(2020)178 [arXiv:2007.14792 [hep-ph]].

[89] B. Kayser and R. E. Shrock, Phys. Lett. B 112, 137-142 (1982) doi:10.1016/0370-2693(82)90314-8

[90] B. Kayser, Phys. Rev. D 26, 1662 (1982) doi:10.1103/PhysRevD.26.1662

[91] B. Kayser and A. S. Goldhaber, Phys. Rev. D 28, 2341 (1983) doi:10.1103/PhysRevD.28.2341

[92] B. Kayser, F. Gibrat-Debu and F. Perrier, World Sci. Lect. Notes Phys. 25, 1-117 (1989)

[93] B. Kayser, [arXiv:hep-ph/9703294 [hep-ph]].

[94] S. Abe et al. [KamLAND-Zen], [arXiv:2203.02139 [hep-ex]].

[95] N. J. Benoit, Y. Kawamura and T. Morozumi, [arXiv:2204.00971 [hep-ph]].

[96] A. Tureanu, Eur. Phys. J. C 80, no.1, 68 (2020) doi:10.1140/epjc/s10052-020-7628-0 [arXiv:1902.01232 [hep- ph]].

[97] M. Blasone and L. Smaldone, Mod. Phys. Lett. A 35, no.38, 2050313 (2020) doi:10.1142/S0217732320503137 [arXiv:2004.04739 [hep-ph]].

[98] H. Umezawa, H. Matsumoto and M. Tachiki, “THERMO FIELD DYNAMICS AND CONDENSED STATES,”

[99] L.E. Ballentine, “Quantum Mechanics A Modern Development,”

[100] R. Haag Z.Naturforsch. 10 (1955) 752 doi:10.1515/zna-1955-9-1014

[101] M. D. Schwartz, “Quantum Field Theory and the Standard Model,”

[102] R.L. Workman et al. [Particle Data Group], PTEP 2022, 083C01 (2022)

[103] M. Aker et al. [KATRIN], Nature Phys. 18, no.2, 160-166 (2022) doi:10.1038/s41567-021-01463-1 [arXiv:2105.08533 [hep-ex]].

[104] A. S. Adam, N. J. Benoit, Y. Kawamura, Y. Mastuo, T. Morozumi, Y. Shimizu, Y. Tokunaga and N. Toyota, doi:10.31526/ACP.BSM- 2021.29 [arXiv:2105.04306 [hep-ph]].

参考文献をもっと見る

全国の大学の
卒論・修論・学位論文

一発検索!

この論文の関連論文を見る