請用此 Handle URI 來引用此文件:
http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/80843完整後設資料紀錄
| DC 欄位 | 值 | 語言 |
|---|---|---|
| dc.contributor.advisor | 黃宇廷(Yu-Tin Huang) | |
| dc.contributor.author | Chun-Yu Liu | en |
| dc.contributor.author | 柳君諭 | zh_TW |
| dc.date.accessioned | 2022-11-24T03:18:45Z | - |
| dc.date.available | 2021-11-08 | |
| dc.date.available | 2022-11-24T03:18:45Z | - |
| dc.date.copyright | 2021-11-08 | |
| dc.date.issued | 2021 | |
| dc.date.submitted | 2021-10-04 | |
| dc.identifier.citation | [1] R. Rattazzi, V. S. Rychkov, E. Tonni and A. Vichi, JHEP 12, 031 (2008) doi:10.1088/1126-6708/2008/12/031 [arXiv:0807.0004 [hep-th]]. [2] D.Simmons-Duffin,doi:10.1142/97898131494410001[arXiv:1602.07982[hep-th]]. [3] D. Poland and D. Simmons-Duffin, Nature Phys. 12, no.6, 535-539 (2016) doi:10.1038/nphys3761 [4] D. Poland, S. Rychkov and A. Vichi, Rev. Mod. Phys. 91, 015002 (2019) doi:10.1103/RevModPhys.91.015002 [arXiv:1805.04405 [hep-th]]. [5] M. F. Paulos, J. Penedones, J. Toledo, B. C. van Rees and P. Vieira, JHEP 11, 133 (2017) doi:10.1007/JHEP11(2017)133 [arXiv:1607.06109 [hep-th]]. [6] M. F. Paulos, J. Penedones, J. Toledo, B. C. van Rees and P. Vieira, JHEP 11, 143 (2017) doi:10.1007/JHEP11(2017)143 [arXiv:1607.06110 [hep-th]]. [7] M. F. Paulos, J. Penedones, J. Toledo, B. C. van Rees and P. Vieira, JHEP 12, 040 (2019) doi:10.1007/JHEP12(2019)040 [arXiv:1708.06765 [hep-th]]. [8] A. Homrich, J. Penedones, J. Toledo, B. C. van Rees and P. Vieira, JHEP 11, 076 (2019) doi:10.1007/JHEP11(2019)076 [arXiv:1905.06905 [hep-th]]. [9] S.D.Chowdhury,A.Gadde,T.Gopalka,I.Halder,L.JanagalandS.Minwalla,JHEP 02, 114 (2020) doi:10.1007/JHEP02(2020)114 [arXiv:1910.14392 [hep-th]]. [10] A.Bose,P.Haldar,A.Sinha,P.SinhaandS.S.Tiwari,[arXiv:2006.12213[hep-th]]. [11] F. Cachazo, S. He and E. Y. Yuan, Phys. Rev. Lett. 113, no.17, 171601 (2014) doi:10.1103/PhysRevLett.113.171601 [arXiv:1307.2199 [hep-th]]. [12]F. Cachazo, S. He and E. Y. Yuan, JHEP 07, 033 (2014) doi:10.1007/JHEP07(2014)033 [arXiv:1309.0885 [hep-th]]. [13]F. Cachazo, S. He and E. Y. Yuan, JHEP 07, 149 (2015) doi:10.1007/JHEP07(2015)149 [arXiv:1412.3479 [hep-th]]. [14] C. R. Mafra, O. Schlotterer and S. Stieberger, Nucl. Phys. B 873, 419-460 doi:10.1016/j.nuclphysb.2013.04.023 [arXiv:1106.2645 [hep-th]]. [15] J. J. M. Carrasco, C. R. Mafra and O. Schlotterer, JHEP 06, 093 doi:10.1007/JHEP06(2017)093 [arXiv:1608.02569 [hep-th]]. [16] C. R. Mafra and O. Schlotterer, JHEP 01, 031 doi:10.1007/JHEP01(2017)031 [arXiv:1609.07078 [hep-th]]. [17] Y. t. Huang, O. Schlotterer and C. Wen, JHEP 09, 155 doi:10.1007/JHEP09(2016)155 [arXiv:1602.01674 [hep-th]]. [18] T. Azevedo, M. Chiodaroli, H. Johansson and O. Schlotterer, JHEP 10, 012 doi:10.1007/JHEP10(2018)012 [arXiv:1803.05452 [hep-th]]. [19] N. Arkani-Hamed, S. He and T. Lam, [arXiv:1912.08707 [hep-th]]. [20] A. Adams, N. Arkani-Hamed, S. Dubovsky, A. Nicolis and R. Rattazzi, JHEP 10, 014 (2006) doi:10.1088/1126-6708/2006/10/014 [arXiv:hep-th/0602178 [hep-th]]. [21] C. Cheung and G. N. Remmen, JHEP 12, 087 (2014) doi:10.1007/JHEP12(2014)087 [arXiv:1407.7865 [hep-th]]. [22] B. Bellazzini, C. Cheung and G. N. Remmen, Phys. Rev. D 93, no.6, 064076 (2016) doi:10.1103/PhysRevD.93.064076 [arXiv:1509.00851 [hep-th]]. [23] C. de Rham, S. Melville, A. J. Tolley and S. Y. Zhou, Phys. Rev. D 96, no.8, 081702 (2017) doi:10.1103/PhysRevD.96.081702 [arXiv:1702.06134 [hep-th]]. [24] C. de Rham, S. Melville and A. J. Tolley, JHEP 04, 083 (2018) doi:10.1007/JHEP04(2018)083 [arXiv:1710.09611 [hep-th]]. [25] W. M. Chen, Y. T. Huang, T. Noumi and C. Wen, Phys. Rev. D 100, no.2, 025016 (2019) doi:10.1103/PhysRevD.100.025016 [arXiv:1901.11480 [hep-th]]. [26] N. Arkani-Hamed, T. C. Huang and Y. T. Huang, [arXiv:2012.15849 [hep-th]]. [27] M. B. Green and C. Wen, JHEP 11, 079 (2019) doi:10.1007/JHEP11(2019)079 [arXiv:1908.08426 [hep-th]]. [28] Plahte, E.. “Symmetry properties of dual tree-graphN-point amplitudes.” Il Nuovo Cimento A (1971-1996) 66 (1970): 713-733. [29] N. E. J. Bjerrum-Bohr, P. H. Damgaard and P. Vanhove, Phys. Rev. Lett. 103 (2009) 161602 doi:10.1103/PhysRevLett.103.161602 [arXiv:0907.1425 [hep-th]]. [30] S. Stieberger, arXiv:0907.2211 [hep-th]. [31] R. H. Boels and T. Hansen, JHEP 06, 054 (2014) doi:10.1007/JHEP06(2014)054 [arXiv:1402.6356 [hep-th]]. [32] D. D. Coon, Phys. Lett. B 29, 669-672 (1969) doi:10.1016/0370-2693(69)90106-3 [33] S. Matsuda, Phys. Rev. 185, 1811-1814 (1969) doi:10.1103/PhysRev.185.1811 [34] N. N. Khuri, Phys. Rev. 185, 1876-1887 (1969) doi:10.1103/PhysRev.185.1876 [35] E. Weimar, “Alternatives to the Veneziano Amplitude,” DESY-74-3. [36] P. G. O. Freund, Phys. Rev. Lett. 20, 235-237 (1968) doi:10.1103/PhysRevLett.20.235 [37] M. Froissart, Phys. Rev. 123, 1053-1057 (1961) doi:10.1103/PhysRev.123.1053 [38] D. J. Gross and P. F. Mende, Phys. Lett. B 197, 129-134 (1987) doi:10.1016/0370-2693(87)90355-8 [39] D. J. Gross and J. L. Manes, Nucl. Phys. B 326, 73-107 (1989) doi:10.1016/0550- 3213(89)90435-5 [40] S. Caron-Huot, Z. Komargodski, A. Sever and A. Zhiboedov, JHEP 10, 026 (2017) doi:10.1007/JHEP10(2017)026 [arXiv:1607.04253 [hep-th]]. [41]E. Perlmutter, JHEP 08, 088 (2015) doi:10.1007/JHEP08(2015)088 [arXiv:1502.07742 [hep-th]]. [42] M. Bianchi, D. Consoli and P. Di Vecchia, [arXiv:2002.05419 [hep-th]]. [43] T. Terasoma, Selberg Integrals and Multiple Zeta Values, Compositio Mathematica 133 (2002) 1–24, [arXiv:9908045[math.AG]]. [44] S. Stieberger, Phys. Rev. Lett. 106 (2011), 111601 doi:10.1103/PhysRevLett.106.111601 [arXiv:0910.0180 [hep-th]]. [45] O. Schlotterer and S. Stieberger, J. Phys. A 46 (2013), 475401 doi:10.1088/1751- 8113/46/47/475401 [arXiv:1205.1516 [hep-th]]. [46] R. Kleiss and H. Kuijf, Nucl. Phys. B 312, 616-644 (1989) doi:10.1016/0550- 3213(89)90574-9 [47] Z. Bern, J. J. M. Carrasco and H. Johansson, Phys. Rev. D 78, 085011 (2008) doi:10.1103/PhysRevD.78.085011 [arXiv:0805.3993 [hep-ph]]. [48] H. Kawai, D. C. Lewellen and S. H. H. Tye, Nucl. Phys. B 269 (1986), 1-23 doi:10.1016/0550-3213(86)90362-7 [49] D. Mazac and M. F. Paulos, JHEP 02, 162 (2019) doi:10.1007/JHEP02(2019)162 [arXiv:1803.10233 [hep-th]]. [50] Brando Bellazzini, Joan Elias Miro, Riccardo Rattazzi, Marc Riembau, and Francesco Riva, to be published. [51] J. J. M. Carrasco, L. Rodina, Z. Yin and S. Zekioglu, [arXiv:1910.12850 [hep-th]]. [52] D. Garfinkle, G. T. Horowitz and A. Strominger, Phys. Rev. D 43, 3140 (1991) Erra- tum: [Phys. Rev. D 45, 3888 (1992)]. doi:10.1103/PhysRevD.43.3140, 10.1103/Phys- RevD.45.3888 [53] N. Arkani-Hamed, L. Motl, A. Nicolis and C. Vafa, JHEP 06, 060 (2007) doi:10.1088/1126-6708/2007/06/060 [arXiv:hep-th/0601001 [hep-th]]. [54] Y. t. Huang, J. Y. Liu, L. Rodina and Y. Wang, JHEP 04, 195 (2021) doi:10.1007/JHEP04(2021)195 [arXiv:2008.02293 [hep-th]]. [55] D. Forde, Phys. Rev. D 75, 125019 (2007) doi:10.1103/PhysRevD.75.125019 [arXiv:0704.1835 [hep-ph]]. [56] N. Arkani-Hamed, F. Cachazo and J. Kaplan, JHEP 1009, 016 (2010) doi:10.1007/JHEP09(2010)016 [arXiv:0808.1446 [hep-th]]. [57] R. Britto, E. Buchbinder, F. Cachazo and B. Feng, Phys. Rev. D 72, 065012 (2005) doi:10.1103/PhysRevD.72.065012 [hep-ph/0503132]. [58] H. Elvang and Y. t. Huang, [arXiv:1308.1697 [hep-th]]. [59] C. Cheung, doi:10.1142/9789813233348 0008 [arXiv:1708.03872 [hep-ph]]. [60] A. Herderschee, S. Koren and T. Trott, JHEP 10, 092 (2019) doi:10.1007/JHEP10(2019)092 [arXiv:1902.07204 [hep-th]]. [61] S.Caron-HuotandZ.Zahraee,JHEP07,179(2019)doi:10.1007/JHEP07(2019)179 [arXiv:1810.04694 [hep-th]]. [62] A. Herderschee, S. Koren and T. Trott, JHEP 08, 107 (2019) doi:10.1007/JHEP08(2019)107 [arXiv:1902.07205 [hep-th]]. [63] G. J. Loges, T. Noumi and G. Shiu, Phys. Rev. D 102, no.4, 046010 (2020) doi:10.1103/PhysRevD.102.046010 [arXiv:1909.01352 [hep-th]]. [64] Y. Kats, L. Motl and M. Padi, JHEP 12, 068 (2007) doi:10.1088/1126- 6708/2007/12/068 [arXiv:hep-th/0606100 [hep-th]]. [65] C. Cheung, J. Liu and G. N. Remmen, JHEP 10, 004 (2018) doi:10.1007/JHEP10(2018)004 [arXiv:1801.08546 [hep-th]]. [66] C. Cheung, J. Liu and G. N. Remmen, Phys. Rev. D 100, no.4, 046003 (2019) doi:10.1103/PhysRevD.100.046003 [arXiv:1903.09156 [hep-th]]. [67] H. S. Reall and J. E. Santos, JHEP 04, 021 (2019) doi:10.1007/JHEP04(2019)021 [arXiv:1901.11535 [hep-th]]. [68] G. Goon and R. Penco, Phys. Rev. Lett. 124, no.10, 101103 (2020) doi:10.1103/PhysRevLett.124.101103 [arXiv:1909.05254 [hep-th]]. [69] A. Adams, N. Arkani-Hamed, S. Dubovsky, A. Nicolis and R. Rattazzi, “Causality, analyticity and an IR obstruction to UV completion,” JHEP 0610, 014 (2006) [hep- th/0602178]. [70] N. Arkani-Hamed, L. Motl, A. Nicolis and C. Vafa, “The String landscape, black holes and gravity as the weakest force,” JHEP 0706, 060 (2007) [hep-th/0601001]. [71] Y. Kats, L. Motl and M. Padi, “Higher-order corrections to mass-charge relation of extremal black holes,” JHEP 0712, 068 (2007) [hep-th/0606100]. [72] H. S. Reall and J. E. Santos, “Higher derivative corrections to Kerr black hole thermodynamics,” JHEP 04, 021 (2019) doi:10.1007/JHEP04(2019)021 [arXiv:1901.11535 [hep-th]]. [73] C. Cheung and G. N. Remmen, “Naturalness and the Weak Gravity Conjecture,” Phys. Rev. Lett. 113, 051601 (2014) [arXiv:1402.2287 [hep-ph]]. [74] N. Arkani-Hamed, T. Huang and Y. Huang, [arXiv:1709.04891 [hep-th]]. [75] G.’tHooftandM.J.G.Veltman,Nucl.Phys.B153,365(1979).doi:10.1016/0550- 3213(79)90605-9 [76] Z. Bern, L. J. Dixon and D. A. Kosower, Phys. Lett. B 302, 299 (1993) Erratum: [Phys. Lett. B 318, 649 (1993)] [77] Z. Bern, L. J. Dixon and D. A. Kosower, Nucl. Phys. B 412, 751 (1994) doi:10.1016/0550-3213(94)90398-0 [78] D. Forde, Phys. Rev. D 75, 125019 (2007) doi:10.1103/PhysRevD.75.125019 [arXiv:0704.1835 [hep-ph]]. [79] N. Arkani-Hamed, F. Cachazo and J. Kaplan, JHEP 1009, 016 (2010) doi:10.1007/JHEP09(2010)016 [arXiv:0808.1446 [hep-th]]. [80] R. Britto, E. Buchbinder, F. Cachazo and B. Feng, Phys. Rev. D 72, 065012 (2005) doi:10.1103/PhysRevD.72.065012 [hep-ph/0503132]. [81] D. A. McGady and L. Rodina, Phys. Rev. D 90, no. 8, 084048 (2014) doi:10.1103/PhysRevD.90.084048 [arXiv:1311.2938 [hep-th]]. [82] P. van Nieuwenhuizen and J. A. M. Vermaseren, Phys. Lett. 65B, 263 (1976). doi:10.1016/0370-2693(76)90178-7 [83] P. van Nieuwenhuizen and J. A. M. Vermaseren, Phys. Rev. D 16, 298 (1977). doi:10.1103/PhysRevD.16.298 [84] M. Fischler, Phys. Rev. D 20, 396 (1979). doi:10.1103/PhysRevD.20.396 [85] D. Garfinkle, G. T. Horowitz and A. Strominger, Phys. Rev. D 43, 3140 (1991) Erra- tum: [Phys. Rev. D 45, 3888 (1992)]. doi:10.1103/PhysRevD.43.3140, 10.1103/Phys- RevD.45.3888 [86] R. Kallosh, A. D. Linde, T. Ortin, A. W. Peet and A. Van Proeyen, Phys. Rev. D 46, 5278 (1992) doi:10.1103/PhysRevD.46.5278 [hep-th/9205027]. [87] T. Ortin, Phys. Rev. D 47, 3136 (1993) doi:10.1103/PhysRevD.47.3136 [hep- th/9208078]. [88] S. Deser and P. van Nieuwenhuizen, Phys. Rev. D 10, 401 (1974) doi:10.1103/PhysRevD.10.401 [89] D. C. Dunbar and P. S. Norridge, Class. Quant. Grav. 14, 351-365 (1997) doi:10.1088/0264-9381/14/2/009 [arXiv:hep-th/9512084 [hep-th]]. [90] A. M. Charles, [arXiv:1906.07734 [hep-th]]. [91] T. Banks, Int. J. Mod. Phys. A 16, 910-921 (2001) doi:10.1142/S0217751X01003998 [arXiv:hep-th/0007146 [hep-th]]. [92] G. Dvali, Fortsch. Phys. 58, 528-536 (2010) doi:10.1002/prop.201000009 [arXiv:0706.2050 [hep-th]]. [93] N. Arkani-Hamed, S. Dimopoulos and S. Kachru, [arXiv:hep-th/0501082 [hep-th]]. [94] S. Dimopoulos, S. Kachru, J. McGreevy and J. G. Wacker, JCAP 08, 003 (2008) doi:10.1088/1475-7516/2008/08/003 [arXiv:hep-th/0507205 [hep-th]]. [95] C. Cheung and G. N. Remmen, Phys. Rev. Lett. 118, no.5, 051601 (2017) doi:10.1103/PhysRevLett.118.051601 [arXiv:1608.02942 [hep-th]]. [96] S. Andriolo, T. C. Huang, T. Noumi, H. Ooguri and G. Shiu, Phys. Rev. D 102, no.4, 046008 (2020) doi:10.1103/PhysRevD.102.046008 [arXiv:2004.13721 [hep-th]]. [97] V. Chandrasekaran, G. N. Remmen and A. Shahbazi-Moghaddam, JHEP 11, 015 (2018) doi:10.1007/JHEP11(2018)015 [arXiv:1804.03153 [hep-th]]. [98] I. Huet, M. Rausch de Traubenberg and C. Schubert, Int. J. Mod. Phys. Conf. Ser. 14, 383-393 (2012) doi:10.1142/S2010194512007507 [arXiv:1112.1049 [hep-th]]. [99] C. Cheung, J. Liu and G. N. Remmen, Phys. Rev. D 100, no.4, 046003 (2019) doi:10.1103/PhysRevD.100.046003 [arXiv:1903.09156 [hep-th]]. [100] D. J. Gross and E. Witten, Nucl. Phys. B 277, 1 (1986) doi:10.1016/0550- 3213(86)90429-3 [101] A. Gruzinov and M. Kleban, Class. Quant. Grav. 24, 3521-3524 (2007) doi:10.1088/0264-9381/24/13/N02 [arXiv:hep-th/0612015 [hep-th]]. [102] C. Herdeiro, E. Radu and K. Uzawa, Phys. Lett. B 818, 136357 (2021) doi:10.1016/j.physletb.2021.136357 [arXiv:2103.00884 [hep-th]]. [103] C. Zhang and S. Y. Zhou, Phys. Rev. Lett. 125, no.20, 201601 (2020) doi:10.1103/PhysRevLett.125.201601 [arXiv:2005.03047 [hep-ph]]. [104] Y. Hamada, T. Noumi and G. Shiu, Phys. Rev. Lett. 123, no.5, 051601 (2019) doi:10.1103/PhysRevLett.123.051601 [arXiv:1810.03637 [hep-th]]. [105] A. P. Porfyriadis and G. N. Remmen, [arXiv:2106.10282 [hep-th]]. [106] O. Aharony and E. Palti, [arXiv:2108.04594 [hep-th]]. | |
| dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/80843 | - |
| dc.description.abstract | "在這篇論文中,我們從兩個不同的出發點討論量子重力給予我們的規範限制。我們將此論文分成兩個部份來討論這兩個出發點。在第一部分,我們研究開弦散射振幅,它同時是時空間中的S-矩陣以及二維全純保角場論。我們先從一個disk積分加上Koba-Nielsen因子出發,在考慮交換對稱以及留數分解的情況下,我們發現該積分可以被展開在SL(2,R)保角區塊。再加入正定條件以及么正性的情況下,我們得知該積分必須為SL(2,R)保角區塊的線性組合,而且Virasoro區塊就落在該解集合的紐折。換句話說,Virasoro區塊正落在邊界上。接著我們考慮低能量的有效場論,在此幺正性展現在耦合存在於EFThedron之中。從Koba-Nielsen窺見,Worldsheet的存在即表示我們的積分具有代數給予的單調關係。我們在有限的微分數底下呈現出單調關係及四維EFThedron兩者對於耦合的條件的交集,這個區域極為細小,在考慮提升為分次數後區域會變得更小。在八個微分數的情形下,我們的區域跟Type-I環形壓實弦論的值zeta(3)誤差約1.5%,zeta(5)誤差約0.2%。這使我們做出推論,我們可以透過單調關係以及EFThedron直接得到四點的開弦散射震幅。第二部分我們考慮弱重力猜想給予有效場論的限制。我們和先回顧愛因斯坦-麥克士威爾以及愛因斯坦-麥克士威爾-脹子理論中帶電的黑洞。我們將給出Reissner-Nordström和GHS黑洞的第一階微擾解,然後討論微擾矩陣的一些性質。帶電黑洞的極值條件會隨著高階微分項的威爾斯係數而改變,我們將會在兩個不同的能量尺度:極紅外區、閥值區,討論威爾斯係數的主要貢獻部分。在極紅外區,我們計算最小耦合,非最小耦合,超重力理論的一圈圖結果。當中我們給出兩個看似會違反若重力猜想的結果。在後續的章節中我們討論閥值區,在此區的威爾森係數主要貢獻是來自於帶有質量的態,我們發現該區域給出的結過皆符合若重力猜想。因此定論最後的結果並沒有違反若重力猜想。" | zh_TW |
| dc.description.provenance | Made available in DSpace on 2022-11-24T03:18:45Z (GMT). No. of bitstreams: 1 U0001-2909202115483500.pdf: 4208222 bytes, checksum: 995a5c50cdc5a11719623fb9621fb599 (MD5) Previous issue date: 2021 | en |
| dc.description.tableofcontents | Acknowledgments iii 中文摘要 v Abstract vii Introduction 1 I String 17 1 Review of String theory 19 1.1 Vertexoperator ............................... 19 1.2 Openstringamplitude............................ 25 1.2.1 Monodromyrelation ........................ 26 1.2.2 Virasoroblock ........................... 26 2 World-sheet positivity 31 2.1 Consistent factorization and the emergence of Virasoro symmetry . . . . 31 2.1.1 Globalblocksfromexchangesymmetry . . . . . . . . . . . . . . 35 2.1.2 Non-negativityandtheVirasoroblock . . . . . . . . . . . . . . . 37 2.2 Themonodromyplane ........................... 42 3 Review of the EFThedron 47 4 Monodromy relation 51 4.1 Intersection of monodromy plane and the EFThedron . . . . . . . . . . . 51 4.2 Theabsenceofisolatedmasslesspoles................... 51 4.3 Combinedconstraints............................ 52 4.4 ClosedstringEFTfromKLT........................ 61 5 Conclusion of Part I 63 II Weak Gravity Conjecture 65 6 Perturbed Black hole 67 6.1 Reissner–Nordstro ̈mblackhole....................... 67 6.2 Dilatonblackhole.............................. 71 6.3 Extremalityandtheaction ......................... 75 7 Weak Gravity Conjecture 79 7.1 Betafunctionsandbubblecuts ....................... 79 7.1.1 Runninginsupergravity ...................... 81 7.1.2 Negative running from nonminimal couplings in non-SUSY theories 83 7.1.3 Causality .............................. 85 7.1.4 UVcompletionandtuning..................... 86 7.2 Actionsandperfectsquares......................... 88 7.2.1 Scalarexamples .......................... 89 7.2.2 Spectralrepresentation....................... 91 7.2.3 Generalizedunitarity........................ 92 7.3 Extremalityandtheaction ......................... 94 8 Outlook 97 A Virasoro block expansion 99 A.1 Virasoroblockcoefficient.......................... 99 A.2 Globalblockdecomposition ........................100 B Ansatz solve Virasoro block coefficients 101 C Bicolor ordered amplitudes 103 C.1 BCJandmonodromyplane.........................103 C.2 Combined constraints for bicolor ordered amplitude . . . . . . . . . 105 C.3 Checkingacorollaryofthemainconjecture . . . . . . . . . . . . . . . . 105 D Supersymmetric spinning polynomial 109 D.1 Reviewofspinningpolynomials ......................111 D.2 N=1Supersymmetry...........................113 D.2.1 TheN=1superpolynomial ...................116 D.3 Extendedsupersymmetry..........................118 D.3.1 ReviewofN=2superspace ...................118 D.3.2 TheN=2superpolynomial ...................120 D.4 ThesupersymmetricEFThedron ......................122 D.4.1 Expansion..............................124 D.5 Conventions.................................125 E The correction of Lagrangian ∆L 127 E.1 Higherorderoperators ...........................127 E.2 ExtremalityandEMAction.........................128 F Unitary Cuts 131 G Positivity and Convexity 133 G.1 DerivationofEq.(7.2.21) .........................133 G.2 Convexityof∆L ..............................134 H Vacuum Polarization 137 I Super-amplitudes in N = 2 141 I.1 Three-pointamplitudes...........................141 I.2 Four-pointamplitudes............................142 Bibliography 143 | |
| dc.language.iso | en | |
| dc.subject | 弱重力猜想 | zh_TW |
| dc.subject | 弦論 | zh_TW |
| dc.subject | 黑洞 | zh_TW |
| dc.subject | 有效場論 | zh_TW |
| dc.subject | 么正性 | zh_TW |
| dc.subject | Effective field theory | en |
| dc.subject | Black Hole | en |
| dc.subject | Weak Gravity Conjecture | en |
| dc.subject | Unitarity | en |
| dc.subject | String theory | en |
| dc.title | 量子重力的規範 | zh_TW |
| dc.title | Constraints from Quantum Gravity | en |
| dc.date.schoolyear | 109-2 | |
| dc.description.degree | 博士 | |
| dc.contributor.oralexamcommittee | 賀培銘(Hsin-Tsai Liu),林豐利(Chih-Yang Tseng),陳江梅,溫文鈺 | |
| dc.subject.keyword | 弦論,有效場論,么正性,弱重力猜想,黑洞, | zh_TW |
| dc.subject.keyword | String theory,Effective field theory,Unitarity,Weak Gravity Conjecture,Black Hole, | en |
| dc.relation.page | 149 | |
| dc.identifier.doi | 10.6342/NTU202103458 | |
| dc.rights.note | 同意授權(限校園內公開) | |
| dc.date.accepted | 2021-10-04 | |
| dc.contributor.author-college | 理學院 | zh_TW |
| dc.contributor.author-dept | 物理學研究所 | zh_TW |
| 顯示於系所單位: | 物理學系 | |
文件中的檔案:
| 檔案 | 大小 | 格式 | |
|---|---|---|---|
| U0001-2909202115483500.pdf 授權僅限NTU校內IP使用(校園外請利用VPN校外連線服務) | 4.11 MB | Adobe PDF |
系統中的文件,除了特別指名其著作權條款之外,均受到著作權保護,並且保留所有的權利。
