Basics of Thermal Field Theory
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Path Integrals in Quantum Mechanics
Path Integrals in Quantum Mechanics Dennis V. Perepelitsa MIT Department of Physics 70 Amherst Ave. Cambridge, MA 02142 Abstract We present the path integral formulation of quantum mechanics and demon- strate its equivalence to the Schr¨odinger picture. We apply the method to the free particle and quantum harmonic oscillator, investigate the Euclidean path integral, and discuss other applications. 1 Introduction A fundamental question in quantum mechanics is how does the state of a particle evolve with time? That is, the determination the time-evolution ψ(t) of some initial | i state ψ(t ) . Quantum mechanics is fully predictive [3] in the sense that initial | 0 i conditions and knowledge of the potential occupied by the particle is enough to fully specify the state of the particle for all future times.1 In the early twentieth century, Erwin Schr¨odinger derived an equation specifies how the instantaneous change in the wavefunction d ψ(t) depends on the system dt | i inhabited by the state in the form of the Hamiltonian. In this formulation, the eigenstates of the Hamiltonian play an important role, since their time-evolution is easy to calculate (i.e. they are stationary). A well-established method of solution, after the entire eigenspectrum of Hˆ is known, is to decompose the initial state into this eigenbasis, apply time evolution to each and then reassemble the eigenstates. That is, 1In the analysis below, we consider only the position of a particle, and not any other quantum property such as spin. 2 D.V. Perepelitsa n=∞ ψ(t) = exp [ iE t/~] n ψ(t ) n (1) | i − n h | 0 i| i n=0 X This (Hamiltonian) formulation works in many cases. -
10. Electroweak Model and Constraints on New Physics
1 10. Electroweak Model and Constraints on New Physics 10. Electroweak Model and Constraints on New Physics Revised March 2020 by J. Erler (IF-UNAM; U. of Mainz) and A. Freitas (Pittsburg U.). 10.1 Introduction ....................................... 1 10.2 Renormalization and radiative corrections....................... 3 10.2.1 The Fermi constant ................................ 3 10.2.2 The electromagnetic coupling........................... 3 10.2.3 Quark masses.................................... 5 10.2.4 The weak mixing angle .............................. 6 10.2.5 Radiative corrections................................ 8 10.3 Low energy electroweak observables .......................... 9 10.3.1 Neutrino scattering................................. 9 10.3.2 Parity violating lepton scattering......................... 12 10.3.3 Atomic parity violation .............................. 13 10.4 Precision flavor physics ................................. 15 10.4.1 The τ lifetime.................................... 15 10.4.2 The muon anomalous magnetic moment..................... 17 10.5 Physics of the massive electroweak bosons....................... 18 10.5.1 Electroweak physics off the Z pole........................ 19 10.5.2 Z pole physics ................................... 21 10.5.3 W and Z decays .................................. 25 10.6 Global fit results..................................... 26 10.7 Constraints on new physics............................... 30 10.1 Introduction The standard model of the electroweak interactions (SM) [1–4] is based on the gauge group i SU(2)×U(1), with gauge bosons Wµ, i = 1, 2, 3, and Bµ for the SU(2) and U(1) factors, respectively, and the corresponding gauge coupling constants g and g0. The left-handed fermion fields of the th νi ui 0 P i fermion family transform as doublets Ψi = − and d0 under SU(2), where d ≡ Vij dj, `i i i j and V is the Cabibbo-Kobayashi-Maskawa mixing [5,6] matrix1. -
Arxiv:1407.4336V2 [Hep-Ph] 10 May 2016 I.Laigtrelo Orcin Otehgsmass Higgs the to Corrections Three-Loop Leading III
Higgs boson mass in the Standard Model at two-loop order and beyond Stephen P. Martin1,2 and David G. Robertson3 1Department of Physics, Northern Illinois University, DeKalb IL 60115 2Fermi National Accelerator Laboratory, P.O. Box 500, Batavia IL 60510 3Department of Physics, Otterbein University, Westerville OH 43081 We calculate the mass of the Higgs boson in the Standard Model in terms of the underlying Lagrangian parameters at complete 2-loop order with leading 3-loop corrections. A computer program implementing the results is provided. The program also computes and minimizes the Standard Model effective po- tential in Landau gauge at 2-loop order with leading 3-loop corrections. Contents I. Introduction 1 II. Higgs pole mass at 2-loop order 2 III. Leading three-loop corrections to the Higgs mass 11 IV. Computer code implementation and numerical results 13 V. Outlook 19 arXiv:1407.4336v2 [hep-ph] 10 May 2016 Appendix: Some loop integral identities 20 References 22 I. INTRODUCTION The Large Hadron Collider (LHC) has discovered [1] a Higgs scalar boson h with mass Mh near 125.5 GeV [2] and properties consistent with the predictions of the minimal Standard Model. At the present time, there are no signals or hints of other new elementary particles. In the case of supersymmetry, the limits on strongly interacting superpartners are model dependent, but typically extend to over an order of magnitude above Mh. It is therefore quite possible, if not likely, that the Standard Model with a minimal Higgs sector exists 2 as an effective theory below 1 TeV, with all other fundamental physics decoupled from it to a very good approximation. -
Relation Between the Pole and the Minimally Subtracted Mass in Dimensional Regularization and Dimensional Reduction to Three-Loop Order
SFB/CPP-07-04 TTP07-04 DESY07-016 hep-ph/0702185 Relation between the pole and the minimally subtracted mass in dimensional regularization and dimensional reduction to three-loop order P. Marquard(a), L. Mihaila(a), J.H. Piclum(a,b) and M. Steinhauser(a) (a) Institut f¨ur Theoretische Teilchenphysik, Universit¨at Karlsruhe (TH) 76128 Karlsruhe, Germany (b) II. Institut f¨ur Theoretische Physik, Universit¨at Hamburg 22761 Hamburg, Germany Abstract We compute the relation between the pole quark mass and the minimally sub- tracted quark mass in the framework of QCD applying dimensional reduction as a regularization scheme. Special emphasis is put on the evanescent couplings and the renormalization of the ε-scalar mass. As a by-product we obtain the three-loop ZOS ZOS on-shell renormalization constants m and 2 in dimensional regularization and thus provide the first independent check of the analytical results computed several years ago. arXiv:hep-ph/0702185v1 19 Feb 2007 PACS numbers: 12.38.-t 14.65.-q 14.65.Fy 14.65.Ha 1 Introduction In quantum chromodynamics (QCD), like in any other renormalizeable quantum field theory, it is crucial to specify the precise meaning of the parameters appearing in the underlying Lagrangian — in particular when higher order quantum corrections are con- sidered. The canonical choice for the coupling constant of QCD, αs, is the so-called modified minimal subtraction (MS) scheme [1] which has the advantage that the beta function, ruling the scale dependence of the coupling, is mass-independent. On the other hand, for a heavy quark besides the MS scheme also other definitions are important — first and foremost the pole mass. -
Euclidean Field Theory
February 2, 2011 Euclidean Field Theory Kasper Peeters & Marija Zamaklar Lecture notes for the M.Sc. in Elementary Particle Theory at Durham University. Copyright c 2009-2011 Kasper Peeters & Marija Zamaklar Department of Mathematical Sciences University of Durham South Road Durham DH1 3LE United Kingdom http://maths.dur.ac.uk/users/kasper.peeters/eft.html [email protected] [email protected] 1 Introducing Euclidean Field Theory5 1.1 Executive summary and recommended literature............5 1.2 Path integrals and partition sums.....................7 1.3 Finite temperature quantum field theory.................8 1.4 Phase transitions and critical phenomena................ 10 2 Discrete models 15 2.1 Ising models................................. 15 2.1.1 One-dimensional Ising model................... 15 2.1.2 Two-dimensional Ising model................... 18 2.1.3 Kramers-Wannier duality and dual lattices........... 19 2.2 Kosterlitz-Thouless model......................... 21 3 Effective descriptions 25 3.1 Characterising phase transitions..................... 25 3.2 Mean field theory.............................. 27 3.3 Landau-Ginzburg.............................. 28 4 Universality and renormalisation 31 4.1 Kadanoff block scaling........................... 31 4.2 Renormalisation group flow........................ 33 4.2.1 Scaling near the critical point................... 33 4.2.2 Critical surface and universality................. 34 4.3 Momentum space flow and quantum field theory........... 35 5 Lattice gauge theory 37 5.1 Lattice action................................. 37 5.2 Wilson loops................................. 38 5.3 Strong coupling expansion and confinement.............. 39 5.4 Monopole condensation.......................... 39 3 4 1 Introducing Euclidean Field Theory 1.1. Executive summary and recommended literature This course is all about the close relation between two subjects which at first sight have very little to do with each other: quantum field theory and the theory of criti- cal statistical phenomena. -
Ads/CFT Correspondence
AdS/CFT Correspondence GEORGE SIOPSIS Department of Physics and Astronomy The University of Tennessee Knoxville, TN 37996-1200 U.S.A. e-mail: [email protected] Notes by James Kettner Fall 2010 ii Contents 1 Path Integral 1 1.1 Quantum Mechanics ........................ 1 1.2 Statistical Mechanics ........................ 3 1.3 Thermodynamics .......................... 4 1.3.1 Canonical ensemble . 4 1.3.2 Microcanonical ensemble . 4 1.4 Field Theory ............................. 4 2 Schwarzschild Black Hole 7 3 Reissner-Nordstrom¨ Black Holes 11 3.1 The holes . 11 3.2 Extremal limit . 13 3.3 Generalizations . 15 3.3.1 Multi-center solution . 15 3.3.2 Arbitrary dimension . 16 3.3.3 Kaluza-Klein reduction . 17 4 Black Branes from String Theory 19 5 Microscopic calculation of Entropy and Hawking Radiation 23 5.1 The hole . 23 5.2 Entropy . 25 5.3 Finite temperature . 27 5.4 Scattering and Hawking radiation . 29 iii iv CONTENTS LECTURE 1 Path Integral 1.1 Quantum Mechanics Set ~ = 1. Given a particle described by coordinates (q, t) with initial and final coor- dinates of (qi, ti) and (qf , tf ), the amplitude of the transition is ∗ hqi, ti | qf , tf i = hψ |qf , tf i = ψ (qf , tf ) . where ψ satisfies the Schrodinger¨ equation ∂ψ 1 ∂2ψ i = − . ∂t 2m ∂q2 Feynman introduced the path integral formalism Z −iS hqi, ti | qf , tf i = [dq] e q(ti)=qi,q(tf )=qf R where S = dtL is the action and L = L(q, q˙) is the Lagrangian, e.g., 1 L = mq˙2 − V (q) 2 We convert to imaginary time via the Wick rotation τ = it so 1 L → − mq˙2 − V (q) ≡ −L 2 E where the derivative is with respect to τ, LE is the total energy (which is bounded Rbelow), and the subscript E stands for Euclidean. -
Quark Mass Renormalization in the MS and RI Schemes up To
ROME1-1198/98 Quark Mass Renormalization in the MS and RI schemes up to the NNLO order Enrico Francoa and Vittorio Lubiczb a Dip. di Fisica, Universit`adegli Studi di Roma “La Sapienza” and INFN, Sezione di Roma, P.le A. Moro 2, 00185 Roma, Italy. b Dip. di Fisica, Universit`adi Roma Tre and INFN, Sezione di Roma, Via della Vasca Navale 84, I-00146 Roma, Italy Abstract We compute the relation between the quark mass defined in the min- imal modified MS scheme and the mass defined in the “Regularization Invariant” scheme (RI), up to the NNLO order. The RI scheme is conve- niently adopted in lattice QCD calculations of the quark mass, since the relevant renormalization constants in this scheme can be evaluated in a non-perturbative way. The NNLO contribution to the conversion factor between the quark mass in the two schemes is found to be large, typically of the same order of the NLO correction at a scale µ ∼ 2 GeV. We also give the NNLO relation between the quark mass in the RI scheme and the arXiv:hep-ph/9803491v1 30 Mar 1998 renormalization group-invariant mass. 1 Introduction The values of quark masses are of great importance in the phenomenology of the Standard Model and beyond. For instance, bottom and charm quark masses enter significantly in the theoretical expressions of inclusive decay rates of heavy mesons, while the strange quark mass plays a crucial role in the evaluation of the K → ππ, ∆I = 1/2, decay amplitude and of the CP-violation parameter ǫ′/ǫ. -
On Mass Interaction Principle
On Mass Interaction Principle Chu-Jun Gu∗ Institute of Theoretical Physics, Grand Genius Group, 100085, Beijing, China 1 2 Abstract This paper proposes mass interaction principle (MIP) as: the particles will be subjected to the random frictionless quantum Brownian motion by the collision of space time particle (STP) prevalent in spacetime. The change in the amount of action of the particles during each collision is an integer multiple of the Planck constant h. The motion of particles under the action of STP is a quantum Markov process. Under this principle, we infer that the statistical inertial mass of a particle is a statistical property that characterizes the difficulty of particle diffusion in spacetime. Starting from this principle, this article has the following six aspects of work: First, we derive the mass-diffusion coefficient uncertainty and the quantized commutation, and derive the most basic coordinate-momentum uncertainty and time-energy uncertainty of quantum mechanics, and then clearly reveal the particle-wave duality, which are properties exhibited by particles collided by STP. Second, we created the three decompositions of particles velocity. The comprehensive property of three velocities deduced the equation of motion of the particle as Schrödinger equation, and made a novel interpretation of Heisenberg’s uncertainty principle and Feynman’s path integral expression. And reexamine the quantum measurement problem, so that the EPR paradox can be explained in a self-consistent manner. Third, we reinterpret the physical origin of quantum spins. Each spacetime random impact not only gives the particle of matter the action of a Planck constant , but also produces the quantum fluctuation properties of the material particles. -
Arxiv:2006.02298V1 [Gr-Qc] 3 Jun 2020
Lorentzian quantum cosmology in novel Gauss-Bonnet gravity from Picard-Lefschetz methods Gaurav Narain a∗ and Hai-Qing Zhang a,b† a Center for Gravitational Physics, Department of Space Science, Beihang University, Beijing 100191, China. b International Research Institute for Multidisciplinary Science, Beihang University, Beijing 100191, China Abstract In this paper we study some aspects of classical and quantum cosmology in the novel-Gauss- Bonnet (nGB) gravity in four space-time dimensions. Starting with a generalised Friedmann- Lemaˆıtre-Robertson-Walker (FLRW) metric respecting homogeneity and isotropicity in arbitrary space-time dimension D, we find the action of theory in four spacetime dimension where the limit D 4 is smoothly obtained after an integration by parts. The peculiar rescaling of Gauss-Bonnet → coupling by factor of D 4 results in a non-trivial contribution to the action. We study the system − of equation of motion to first order nGB coupling. We then go on to compute the transition probability from one 3-geometry to another directly in Lorentzian signature. We make use of combination of WKB approximation and Picard-Lefschetz (PL) theory to achieve our aim. PL theory allows to analyse the path-integral directly in Lorentzian signature without doing Wick rotation. Due to complication caused by non-linear nature of action, we compute the transition amplitude to first order in nGB coupling. We find non-trivial correction coming from the nGB coupling to the transition amplitude, even if the analysis was done perturbatively. We use this result to investigate the case of classical boundary conditions. arXiv:2006.02298v1 [gr-qc] 3 Jun 2020 ∗ [email protected] † [email protected] 1 I. -
MS-On-Shell Quark Mass Relation up to Four Loops in QCD and a General SU
DESY 16-106, TTP16-023 MS-on-shell quark mass relation up to four loops in QCD and a general SU(N) gauge group Peter Marquarda, Alexander V. Smirnovb, Vladimir A. Smirnovc, Matthias Steinhauserd, David Wellmannd (a) Deutsches Elektronen-Synchrotron, DESY 15738 Zeuthen, Germany (b) Research Computing Center, Moscow State University 119991, Moscow, Russia (c) Skobeltsyn Institute of Nuclear Physics of Moscow State University 119991, Moscow, Russia (d) Institut f¨ur Theoretische Teilchenphysik, Karlsruhe Institute of Technology (KIT) 76128 Karlsruhe, Germany Abstract We compute the relation between heavy quark masses defined in the modified minimal subtraction and the on-shell schemes. Detailed results are presented for all coefficients of the SU(Nc) colour factors. The reduction of the four-loop on- shell integrals is performed for a general QCD gauge parameter. Altogether there are about 380 master integrals. Some of them are computed analytically, others with high numerical precision using Mellin-Barnes representations, and the rest numerically with the help of FIESTA. We discuss in detail the precise numerical evaluation of the four-loop master integrals. Updated relations between various arXiv:1606.06754v2 [hep-ph] 14 Nov 2016 short-distance masses and the MS quark mass to next-to-next-to-next-to-leading order accuracy are provided for the charm, bottom and top quarks. We discuss the dependence on the renormalization and factorization scale. PACS numbers: 12.38.Bx, 12.38.Cy, 14.65.Fy, 14.65.Ha 1 Introduction Quark masses are fundamental parameters of Quantum Chromodynamics (QCD) and thus it is mandatory to determine their numerical values as precisely as possible. -
Higgs Boson Mass and New Physics Arxiv:1205.2893V1
Higgs boson mass and new physics Fedor Bezrukov∗ Physics Department, University of Connecticut, Storrs, CT 06269-3046, USA RIKEN-BNL Research Center, Brookhaven National Laboratory, Upton, NY 11973, USA Mikhail Yu. Kalmykovy Bernd A. Kniehlz II. Institut f¨urTheoretische Physik, Universit¨atHamburg, Luruper Chaussee 149, 22761, Hamburg, Germany Mikhail Shaposhnikovx Institut de Th´eoriedes Ph´enom`enesPhysiques, Ecole´ Polytechnique F´ed´eralede Lausanne, CH-1015 Lausanne, Switzerland May 15, 2012 Abstract We discuss the lower Higgs boson mass bounds which come from the absolute stability of the Standard Model (SM) vacuum and from the Higgs inflation, as well as the prediction of the Higgs boson mass coming from asymptotic safety of the SM. We account for the 3-loop renormalization group evolution of the couplings of the Standard Model and for a part of two-loop corrections that involve the QCD coupling αs to initial conditions for their running. This is one step above the current state of the art procedure (\one-loop matching{two-loop running"). This results in reduction of the theoretical uncertainties in the Higgs boson mass bounds and predictions, associated with the Standard Model physics, to 1−2 GeV. We find that with the account of existing experimental uncertainties in the mass of the top quark and αs (taken at 2σ level) the bound reads MH ≥ Mmin (equality corresponds to the asymptotic safety prediction), where Mmin = 129 ± 6 GeV. We argue that the discovery of the SM Higgs boson in this range would be in arXiv:1205.2893v1 [hep-ph] 13 May 2012 agreement with the hypothesis of the absence of new energy scales between the Fermi and Planck scales, whereas the coincidence of MH with Mmin would suggest that the electroweak scale is determined by Planck physics. -
Pole Mass, Width, and Propagators of Unstable Fermions
DESY 08-001 ISSN 0418-9833 NYU-TH/08/01/04 January 2008 Pole Mass, Width, and Propagators of Unstable Fermions Bernd A. Kniehl∗ II. Institut f¨ur Theoretische Physik, Universit¨at Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany Alberto Sirlin† Department of Physics, New York University, 4 Washington Place, New York, New York 10003, USA Abstract The concepts of pole mass and width are extended to unstable fermions in the general framework of parity-nonconserving gauge theories, such as the Standard Model. In contrast with the conventional on-shell definitions, these concepts are gauge independent and avoid severe unphysical singularities, properties of great importance since most fundamental fermions in nature are unstable particles. Gen- eral expressions for the unrenormalized and renormalized dressed propagators of unstable fermions and their field-renormalization constants are presented. PACS: 11.10.Gh, 11.15.-q, 11.30.Er, 12.15.Ff arXiv:0801.0669v1 [hep-th] 4 Jan 2008 ∗Electronic address: [email protected]. †Electronic address: [email protected]. 1 The conventional definitions of mass and width of unstable bosons are 2 2 2 mos = m0 + Re A(mos), (1) 2 Im A(mos) mosΓos = − ′ 2 , (2) 1 − Re A (mos) where m0 is the bare mass and A(s) is the self-energy in the scalar case and the transverse self-energy in the vector boson case. The subscript os means that Eqs. (1) and (2) define the on-shell mass and the on-shell width, respectively. However, it was shown in Ref. [1] that, in the context of gauge theories, mos and Γos are gauge dependent in next-to-next-to-leading order.