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| DC 欄位 | 值 | 語言 |
|---|---|---|
| dc.contributor.advisor | 陳丕燊(Pisin Chen) | |
| dc.contributor.author | Kuan-Yu Chen | en |
| dc.contributor.author | 陳冠宇 | zh_TW |
| dc.date.accessioned | 2022-11-23T09:07:10Z | - |
| dc.date.available | 2021-10-04 | |
| dc.date.available | 2022-11-23T09:07:10Z | - |
| dc.date.copyright | 2021-10-04 | |
| dc.date.issued | 2021 | |
| dc.date.submitted | 2021-08-31 | |
| dc.identifier.citation | [1] R. J. Adler, P. Chen, and D. I. Santiago. The Generalized uncertainty principle and black hole remnants. Gen. Rel. Grav., 33:2101–2108, 2001. [2] A. Almheiri, N. Engelhardt, D. Marolf, and H. Maxfield. The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole. JHEP, 12:063, 2019. [3] A. Almheiri, R. Mahajan, J. Maldacena, and Y. Zhao. The Page curve of Hawking radiation from semiclassical geometry. JHEP, 03:149, 2020. [4] A. Almheiri, D. Marolf, J. Polchinski, and J. Sully. Black Holes: Complementarity or Firewalls? JHEP, 02:062, 2013. [5] J. M. Bardeen, B. Carter, and S. W. Hawking. The Four laws of black hole mechanics. Commun. Math. Phys., 31:161–170, 1973. [6] E. Batista and S. Majid. Noncommutative geometry of angular momentum space U(su(2)). J. Math. Phys., 44:107–137, 2003. [7] J. D. Bekenstein. Black holes and entropy. Phys. Rev. D, 7:2333–2346, 1973. [8] D. Carney, L. Chaurette, D. Neuenfeld, and G. W. Semenoff. Infrared quantum information. Phys. Rev. Lett., 119(18):180502, 2017. [9] P. Chen and G. Mourou. Accelerating Plasma Mirrors to Investigate Black Hole Information Loss Paradox. Phys. Rev. Lett., 118(4):045001, 2017. [10] P. Chen, Y. C. Ong, and D.h. Yeom. Black Hole Remnants and the Information Loss Paradox. Phys. Rept., 603:1–45, 2015. [11] H.W. Chiang, Y.C. Hu, and P. Chen. Quantization of spacetime based on a spacetime interval operator. Phys. Rev. D, 93(8):084043, 2016. [12] H.W. Chiang, Y.H. Kung, and P. Chen. Modification to the Hawking temperature of a dynamical black hole by a flowinduced supertranslation. 4 2020. [13] P. T. Chrusciel, J. Lopes Costa, and M. Heusler. Stationary Black Holes: Uniqueness and Beyond. Living Rev. Rel., 15:7, 2012. [14] M.Z. Chung, Y.T. Huang, J.W. Kim, and S. Lee. The simplest massive Smatrix: from minimal coupling to Black Holes. JHEP, 04:156, 2019. [15] A. Connes. Gravity coupled with matter and foundation of noncommutative geometry. Commun. Math. Phys., 182:155–176, 1996. [16] J. S. Cotler, G. GurAri, M. Hanada, J. Polchinski, P. Saad, S. H. Shenker, D. Stanford, A. Streicher, and M. Tezuka. Black Holes and Random Matrices. JHEP, 05:118, 2017. [Erratum: JHEP 09, 002 (2018)]. [17] S. Doplicher, K. Fredenhagen, and J. E. Roberts. The Quantum structure of spacetime at the Planck scale and quantum fields. Commun. Math. Phys., 172:187 220, 1995. [18] E. E. Flanagan. OrderUnity Correction to Hawking Radiation. Phys. Rev. Lett., 127(4):041301, 2021. [19] G. W. Gibbons and S. W. Hawking. Action Integrals and Partition Functions in Quantum Gravity. Phys. Rev. D, 15:2752–2756, 1977. [20] A. Hashimoto and N. Itzhaki. Noncommutative YangMills and the AdS / CFT correspondence. Phys. Lett. B, 465:142–147, 1999. [21] S. W. Hawking. Particle Creation by Black Holes. Commun. Math. Phys., 43:199 220, 1975. [,167(1975)]. [22] S. W. Hawking. Breakdown of Predictability in Gravitational Collapse. Phys. Rev. D, 14:2460–2473, 1976. [23] S. W. Hawking, M. J. Perry, and A. Strominger. Soft Hair on Black Holes. Phys. Rev. Lett., 116(23):231301, 2016. [24] S. W. Hawking, M. J. Perry, and A. Strominger. Superrotation Charge and Supertranslation Hair on Black Holes. JHEP, 05:161, 2017. [25] P. Hayden and J. Preskill. Black holes as mirrors: Quantum information in random subsystems. JHEP, 09:120, 2007. [26] M. Hotta, Y. Nambu, and K. Yamaguchi. SoftHairEnhanced Entanglement Beyond Page Curves in a Blackhole Evaporation Qubit Model. Phys. Rev. Lett., 120(18):181301, 2018. [27] M. Hotta, R. Schützhold, and W. G. Unruh. Partner particles for moving mirror radiation and black hole evaporation. Phys. Rev. D, 91(12):124060, 2015. [28] J. Hwang, D. S. Lee, D. Nho, J. Oh, H. Park, D.h. Yeom, and H. Zoe. Page curves for tripartite systems. Class. Quant. Grav., 34(14):145004, 2017. [29] J. Maldacena and L. Susskind. Cool horizons for entangled black holes. Fortsch. Phys., 61:781–811, 2013. [30] S. D. Mathur. The Information paradox: A Pedagogical introduction. Class. Quant. Grav., 26:224001, 2009. [31] D. N. Page. Information in black hole radiation. Phys. Rev. Lett., 71:3743–3746, 1993. [32] M. K. Parikh. A Secret tunnel through the horizon. Int. J. Mod. Phys. D, 13:2351– 2354, 2004. [33] S. Pasterski and H. Verlinde. HPS meets AMPS: How Soft Hair Dissolves the Firewall. 12 2020. [34] G. Penington, S. H. Shenker, D. Stanford, and Z. Yang. Replica wormholes and the black hole interior. 11 2019. [35] S. Ryu and T. Takayanagi. Holographic derivation of entanglement entropy from AdS/CFT. Phys. Rev. Lett., 96:181602, 2006. [36] J. Steinhauer. Observation of selfamplifying Hawking radiation in an analog blackhole laser. Nature Phys., 10:864, 2014. [37] A. Strominger. On BMS Invariance of Gravitational Scattering. JHEP, 07:152, 2014. [38] L. Susskind, L. Thorlacius, and J. Uglum. The Stretched horizon and black hole complementarity. Phys. Rev. D, 48:3743–3761, 1993. [39] W. G. Unruh. Notes on black hole evaporation. Phys. Rev. D, 14:870, 1976. [40] W. G. Unruh. Experimental black hole evaporation. Phys. Rev. Lett., 46:1351–1353, 1981. [41] W. G. Unruh and R. M. Wald. On evolution laws taking pure states to mixed states in quantum field theory. Phys. Rev. D, 52:2176–2182, 1995. [42] W. G. Unruh and R. M. Wald. Information Loss. Rept. Prog. Phys., 80(9):092002, 2017. [43] E. P. Verlinde. On the Origin of Gravity and the Laws of Newton. JHEP, 04:029, 2011. [44] R. M. Wald. Black hole entropy is the Noether charge. Phys. Rev., D48(8):R3427– R3431, 1993. [45] S. Weinberg and E. Witten. Limits on Massless Particles. Phys. Lett. B, 96:59–62, 1980. | |
| dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/79675 | - |
| dc.description.abstract | 我們介紹了一個可以描述自洽的黑洞蒸發圖像所需的必要特徵的泛用模型。然而儘管新模型的解釋能力十分強大,我們還是展示出了在本模型下黑洞必然是會漏出資訊的。一個么正的黑洞蒸發過程必須包含一個'隱藏區域'-一種在事件視界上隱密的零能量衰減蒸發過程,來暫時儲存資訊。除此之外,黑洞的微觀態密度與宏觀的熱力學性質在確立最終爆發與零能量極點可相互連結,與正比於黑洞蒸發末時貝肯斯坦上限對應的熵之紫外界限時,兩者可以相互關聯。 | zh_TW |
| dc.description.provenance | Made available in DSpace on 2022-11-23T09:07:10Z (GMT). No. of bitstreams: 1 U0001-3008202119373500.pdf: 1007018 bytes, checksum: 6b460291cfc94316eb7e3f311423a254 (MD5) Previous issue date: 2021 | en |
| dc.description.tableofcontents | Verification Letter from the Oral Examination Committee i Acknowledgements iii 摘要v Abstract vii Contents ix List of Figures xi Chapter 1 Introduction 1 Chapter 2 CCCY Horizon Model 5 2.1 Setup . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 2.2 Quanta counting and Bekenstein’s bound . . . . . . . . . . . . . . . 7 2.3 Dimensional analysis and the extended Bekenstein’s law . . . . . . . 9 Chapter 3 Statistical analysis 13 3.1 Dimensionality and noncommutativity of the configuration space . . 15 Chapter 4 Conclusion 17 References 19 | |
| dc.language.iso | en | |
| dc.title | 自第一原理架構泛用么正黑洞蒸發模型之分析 | zh_TW |
| dc.title | Analysis of generic unitary black-hole evaporation models from first principles | en |
| dc.date.schoolyear | 109-2 | |
| dc.description.degree | 碩士 | |
| dc.contributor.oralexamcommittee | 黃宇廷(Hsin-Tsai Liu),陳哲佑(Chih-Yang Tseng) | |
| dc.subject.keyword | 黑洞蒸發,資訊遺失悖論,量子位元模型,黑洞熵,軟髮, | zh_TW |
| dc.subject.keyword | Black hole evaporation,Information loss paradox,Qubit model,Black hole entropy,Soft hair, | en |
| dc.relation.page | 23 | |
| dc.identifier.doi | 10.6342/NTU202102861 | |
| dc.rights.note | 同意授權(全球公開) | |
| dc.date.accepted | 2021-09-01 | |
| 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 | |
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