riversongs Posted March 12 Report Share Posted March 12 Free Download Qft In Curved Spacetime - Hawking Radiation, Unruh EffectPublished: 3/2025MP4 | Video: h264, 1920x1080 | Audio: AAC, 44.1 KHzLanguage: English | Size: 14.24 GB | Duration: 16h 56mQuantum Field Theory in curved spacetime, Hawking radiation, Unruh effect, quantum corrections to General RelativityWhat you'll learnUnderstand Quantum Fields in Curved Spacetime: Learn how quantum fields are formulated in non-Minkowskian geometries, explore vacuum statesAnalyze Black Hole Thermodynamics and Radiation: Derive and interpret Hawking radiation, study black hole entropy, and examine evaporation processesMaster Mathematical Techniques for Quantum Corrections to Gravity: Develop proficiency in path integrals, heat kernel methods, zeta function regularizationApply QFT in Curved Spacetime to Modern Research Topics: Investigate the Unruh effect, semiclassical gravity, quantum corrections to General RelativityExplore the Role of Bogolyubov Transformations and Vacuum States: Understand how Bogolyubov coefficients relate different vacuum states, analyze Rindler vacuumDevelop a Strong Foundation in Lorentz and Poincaré Representations: apply these techniques to derive the DIrac equation in curved spacetimeRequirementsBackground in Quantum Field Theory and General Relativity: Students should have a solid understanding of QFT and GR, including classical field theory, the Klein-Gordon equation, and the basics of curved spacetime.Mathematical Proficiency: Familiarity with functional analysis, differential geometry, and advanced calculus is strongly recommended, as these mathematical tools are extensively used throughout the course.Exposure to Path Integrals and Operator Formalism: While a full mastery is not required, prior exposure to the path integral formulation and operator-based quantization methods in quantum mechanics and QFT will be beneficial.DescriptionThis advanced course examines the interface of quantum field theory (QFT) and general relativity, focusing on the theoretical and mathematical structures that govern quantum fields in curved spacetime. The course is intended for graduate students, researchers, as well as professionals in theoretical physics.The syllabus includes the following key topics (not necessarily in this order):Foundations of QFT in Curved SpacetimeDefinition of quantum fields in non-Minkowskian geometries.Vacuum states, particle creation, and the semiclassical approach.Hawking RadiationDerivation and analysis of black hole radiation.Implications for black hole thermodynamics and entropy.Black hole lifetime and evaporation processesInsights from the holographic principle and Loop Quantum GravityThe Unruh EffectExamination of vacuum fluctuations as perceived by uniformly accelerated observers.Theoretical connection to the Rindler horizon and thermal effects.Rindler and Minkowski vacua, and the role of Bogolyubov coefficientsConnection between acceleration, temperature, and entropyMathematical Framework for the Calculation of Quantum Corrections to GravityPath integral formulation and its application to curved spacetimeHeat kernel methods, zeta function regularization, and renormalizationEuclidean quantum gravity and effective action approachesLorentz and Poincaré group representations in curved spacetimeApplications to Quantum Gravity & CosmologyQuantum corrections to General Relativity from effective field theoryScalar fields in expanding universes and inflationary modelsCasimir force, semiclassical gravity, and emergent spacetime modelsBy the end of the course, students will develop a thorough understanding of the core theoretical principles of QFT in curved spacetime, as well as their implications for fundamental physics. The course will equip participants with the tools necessary to engage in more advanced research in quantum gravity, black hole physics, and cosmology.Prerequisites:Participants should have a solid foundation in QFT and general relativity. Familiarity with advanced mathematical methods, including functional analysis and differential geometry, is strongly recommended. However, the first section recalls those relevant concepts of QFT, which are used extensively throughout the course.Course Format:The course is structured around "formal" lectures (aiming to stimulate physical and mathematical intuition), and critical discussions of seminal and contemporary research literature. It aims to provide a rigorous and comprehensive understanding of the subject.OverviewSection 1: Introduction to the courseLecture 1 General introductory videoLecture 2 What is Quantum Field Theory in curved spacetime?Lecture 3 Book resources (which are NOT mandatory to follow the course)Lecture 4 More information about the content of the courseSection 2: Recap on Quantum Field Theory for scalar fieldsLecture 5 introduction to the section dedicated to the recap on QFTLecture 6 Reconciling quantum mechanics and Special RelativityLecture 7 Review of Classical Field Theory part 1Lecture 8 Review of Classical Field Theory part 2Lecture 9 Klein Gordon equation derived from Classical field theoryLecture 10 Quantization of a Classical Field part 1Lecture 11 Quantization of a Classical Field part 2Lecture 12 Derivation of the spectrum of the Hamiltonian part 1Lecture 13 Expression of the energy momentum tensor in Field TheoryLecture 14 Annihilation and creation operators to determine the spectrum of the HamiltonianLecture 15 Ground state and construction of states with a certain number of quantaLecture 16 Definition of the number operatorLecture 17 Number operator acting on a two-particle stateLecture 18 Invariant volume element in QFTSection 3: Unruh effect and Hawking radiationLecture 19 lightcone coordinatesLecture 20 scalar field in curved space, Rindler vacuum, Minkowski vacuumLecture 21 Bogolyubov transformationsLecture 22 Coefficients in the Bogolyubov transformationsLecture 23 Bogolyubov normalization conditionLecture 24 Unruh effectLecture 25 Hawking radiationLecture 26 Thermodynamics of black holesLecture 27 The lifetime of blackholesLecture 28 Holographic principle and emergent gravityLecture 29 Black holes from the perspective of Loop Quantum GravityLecture 30 The connection between General Relativity and thermodynamicsLecture 31 Classical scalar field in an expanding universeLecture 32 Appendix on the Planck lengthSection 4: Recap on Path IntegralsLecture 33 Derivation of the path integralLecture 34 Mathematical and physical intuition behind the path integralLecture 35 Heuristic derivation of the path integral from classical field theoryLecture 36 A different perspective: from the path integral to the Schrodinger equationLecture 37 Double Slit Experiment Analysis Using Path Integrals (implementation in MATLAB)Lecture 38 Double-Slit Experiment using Path Integrals: some more physical considerationsLecture 39 Appendix: Solving an Integral from Feynman's Book on Path IntegralsSection 5: Difficulties in the quantization of gravityLecture 40 Semiclassical gravityLecture 41 Why Quantum Gravity is hardLecture 42 Some possible approaches to Quantum Gravity: qualitative considerationsSection 6: Quantum effects of fields in vacuum: Casimir effectLecture 43 Quantum effects in vacuum: Casimir force in 1+1 dimensionsLecture 44 Speculative considerations on Casimir effect and possible gravitational effectsSection 7: Quantum effects in gravity: path integrals in curved spacetime, Heat kernelLecture 45 Euclidean action for a scalar field coupled to gravityLecture 46 Effective action as a functional determinantLecture 47 Reformulation of the eigenvalue problem of a scalar field coupled to gravityLecture 48 Zeta function of a mathematical operatorLecture 49 Heat kernel and quantum corrections to General RelativityLecture 50 Calculation of the Heat kernel in curved space part 1Lecture 51 Calculation of the Heat kernel in curved space part 2Lecture 52 Calculation of the Heat kernel in curved space part 3: matrix elements of K0Lecture 53 Calculation of the Heat kernel in curved space part 4: matrix elements of K1Lecture 54 Calculation of the Heat kernel in curved space part 5: corrections to GRLecture 55 Appendix: why can we make anything uself out of divergences in physics?Section 8: Lorentz group, representations, spinors, Dirac equation in curved spacetimeLecture 56 Lorentz and Poincare groups, representations, angular momentum, Lie algebrasLecture 57 Derivation of the Lorentz Lie algebraLecture 58 Transformation of a vector field according to the Lorentz algebraLecture 59 Transformation of a spinor field derived by generalizing a vector fieldLecture 60 The generators of the transformation of a vector satisfy the Lorentz algebraLecture 61 The generators of the transformation of a spinor satisfy the Lorentz algebraLecture 62 Derivation of the commutator of angular momentum from the Lorentz Lie algebraLecture 63 Tetrads and Dirac equation in curved spacetimeLecture 64 Appendix on the exponential of a matrixGraduate Students & Researchers in Theoretical Physics: This course is designed for students pursuing master's or PhD-level studies in quantum field theory, general relativity, or related fields. 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