Gravity's Quantum Side
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The Future of Fundamental Physics
The Future of Fundamental Physics Nima Arkani-Hamed Abstract: Fundamental physics began the twentieth century with the twin revolutions of relativity and quantum mechanics, and much of the second half of the century was devoted to the con- struction of a theoretical structure unifying these radical ideas. But this foundation has also led us to a number of paradoxes in our understanding of nature. Attempts to make sense of quantum mechanics and gravity at the smallest distance scales lead inexorably to the conclusion that space- Downloaded from http://direct.mit.edu/daed/article-pdf/141/3/53/1830482/daed_a_00161.pdf by guest on 23 September 2021 time is an approximate notion that must emerge from more primitive building blocks. Further- more, violent short-distance quantum fluctuations in the vacuum seem to make the existence of a macroscopic world wildly implausible, and yet we live comfortably in a huge universe. What, if anything, tames these fluctuations? Why is there a macroscopic universe? These are two of the central theoretical challenges of fundamental physics in the twenty-½rst century. In this essay, I describe the circle of ideas surrounding these questions, as well as some of the theoretical and experimental fronts on which they are being attacked. Ever since Newton realized that the same force of gravity pulling down on an apple is also responsible for keeping the moon orbiting the Earth, funda- mental physics has been driven by the program of uni½cation: the realization that seemingly disparate phenomena are in fact different aspects of the same underlying cause. By the mid-1800s, electricity and magnetism were seen as different aspects of elec- tromagnetism, and a seemingly unrelated phenom- enon–light–was understood to be the undulation of electric and magnetic ½elds. -
Report of Contributions
2016 CAP Congress / Congrès de l’ACP 2016 Report of Contributions https://indico.cern.ch/e/CAP2016 2016 CAP Congr … / Report of Contributions **WITHDRAWN** Nanoengineeri … Contribution ID: 980 Type: Oral (Non-Student) / orale (non-étudiant) **WITHDRAWN** Nanoengineering materials: a bottom-up approach towards understanding long outstanding challenges in condensed matter science Thursday, 16 June 2016 08:30 (15 minutes) Chemists have made tremendous advances in synthesizing a variety of nanostructures with control over their size, shape, and chemical composition. Plus, it is possible to control their assembly and to make macroscopic materials. Combined, these advances suggest an opportunity to “nanoengineer” materials ie controllably fabricate materials from the nanoscale up with a wide range of controlled and potentially even new behaviours. Our group has been exploring this opportunity, and has found a rich range of material elec- tronic behaviours that even simple nano-building blocks can generate, e.g. single electron effects, metal-insulator transitions, semiconductor transistor-like conductance gating, and, most recently, strongly correlated electronic behaviour. The latter is particularly exciting. Strongly correlated electrons are known to lie at the heart of some of the most exotic, widely studied and still out- standing challenges in condensed matter science (e.g. high Tc superconductivity in the cuprates and others). The talk will survey both new insights and new opportunities that arise as a result of usingthis nanoengineering -
Large-D Behavior of the Feynman Amplitudes for a Just-Renormalizable Tensorial Group Field Theory
PHYSICAL REVIEW D 103, 085006 (2021) Large-d behavior of the Feynman amplitudes for a just-renormalizable tensorial group field theory † Vincent Lahoche1,* and Dine Ousmane Samary 1,2, 1Commissariatal ` ’Énergie Atomique (CEA, LIST), 8 Avenue de la Vauve, 91120 Palaiseau, France 2Facult´e des Sciences et Techniques (ICMPA-UNESCO Chair), Universit´ed’Abomey- Calavi, 072 BP 50, Benin (Received 22 December 2020; accepted 22 March 2021; published 16 April 2021) This paper aims at giving a novel approach to investigate the behavior of the renormalization group flow for tensorial group field theories to all order of the perturbation theory. From an appropriate choice of the kinetic kernel, we build an infinite family of just-renormalizable models, for tensor fields with arbitrary rank d. Investigating the large d-limit, we show that the self-energy melonic amplitude is decomposed as a product of loop-vertex functions depending only on dimensionless mass. The corresponding melonic amplitudes may be mapped as trees in the so-called Hubbard-Stratonivich representation, and we show that only trees with edges of different colors survive in the large d-limit. These two key features allow to resum the perturbative expansion for self energy, providing an explicit expression for arbitrary external momenta in terms of Lambert function. Finally, inserting this resummed solution into the Callan-Symanzik equations, and taking into account the strong relation between two and four point functions arising from melonic Ward- Takahashi identities, we then deduce an explicit expression for relevant and marginal β-functions, valid to all orders of the perturbative expansion. By investigating the solutions of the resulting flow, we conclude about the nonexistence of any fixed point in the investigated region of the full phase space. -
Quantum Field Theory*
Quantum Field Theory y Frank Wilczek Institute for Advanced Study, School of Natural Science, Olden Lane, Princeton, NJ 08540 I discuss the general principles underlying quantum eld theory, and attempt to identify its most profound consequences. The deep est of these consequences result from the in nite number of degrees of freedom invoked to implement lo cality.Imention a few of its most striking successes, b oth achieved and prosp ective. Possible limitation s of quantum eld theory are viewed in the light of its history. I. SURVEY Quantum eld theory is the framework in which the regnant theories of the electroweak and strong interactions, which together form the Standard Mo del, are formulated. Quantum electro dynamics (QED), b esides providing a com- plete foundation for atomic physics and chemistry, has supp orted calculations of physical quantities with unparalleled precision. The exp erimentally measured value of the magnetic dip ole moment of the muon, 11 (g 2) = 233 184 600 (1680) 10 ; (1) exp: for example, should b e compared with the theoretical prediction 11 (g 2) = 233 183 478 (308) 10 : (2) theor: In quantum chromo dynamics (QCD) we cannot, for the forseeable future, aspire to to comparable accuracy.Yet QCD provides di erent, and at least equally impressive, evidence for the validity of the basic principles of quantum eld theory. Indeed, b ecause in QCD the interactions are stronger, QCD manifests a wider variety of phenomena characteristic of quantum eld theory. These include esp ecially running of the e ective coupling with distance or energy scale and the phenomenon of con nement. -
Semiclassical Gravity and Quantum De Sitter
Semiclassical gravity and quantum de Sitter Neil Turok Perimeter Institute Work with J. Feldbrugge, J-L. Lehners, A. Di Tucci Credit: Pablo Carlos Budassi astonishing simplicity: just 5 numbers Measurement Error Expansion rate: 67.8±0.9 km s−1 Mpc−1 1% today (Temperature) 2.728 ± 0.004 K .1% (Age) 13.799 ±0.038 bn yrs .3% Baryon-entropy ratio 6±.1x10-10 1% energy Dark matter-baryon ratio 5.4± 0.1 2% Dark energy density 0.69±0.006 x critical 2% Scalar amplitude 4.6±0.006 x 10-5 1% geometry Scalar spectral index -.033±0.004 12% ns (scale invariant = 0) A dns 3 4 gw consistent +m 's; but Ωk , 1+ wDE , d ln k , δ , δ ..,r = A with zero ν s Nature has found a way to create a huge hierarchy of scales, apparently more economically than in any current theory A fascinating situation, demanding new ideas One of the most minimal is to revisit quantum cosmology The simplest of all cosmological models is de Sitter; interesting both for today’s dark energy and for inflation quantum cosmology reconsidered w/ S. Gielen 1510.00699, Phys. Rev. Le+. 117 (2016) 021301, 1612.0279, Phys. Rev. D 95 (2017) 103510. w/ J. Feldbrugge J-L. Lehners, 1703.02076, Phys. Rev. D 95 (2017) 103508, 1705.00192, Phys. Rev. Le+, 119 (2017) 171301, 1708.05104, Phys. Rev. D, in press (2017). w/A. Di Tucci, J. Feldbrugge and J-L. Lehners , in PreParaon (2017) Wheeler, Feynman, Quantum geometrodynamics De Wi, Teitelboim … sum over final 4-geometries 3-geometry (4) Σ1 gµν initial 3-geometry Σ0 fundamental object: Σ Σ ≡ 1 0 Feynman propagator 1 0 Basic object: phase space Lorentzian path integral 2 2 i 2 i (3) i j ADM : ds ≡ (−N + Ni N )dt + 2Nidtdx + hij dx dx Σ1 i (3) (3) i S 1 0 = DN DN Dh Dπ e ! ∫ ∫ ∫ ij ∫ ij Σ0 1 S = dt d 3x(π (3)h!(3) − N H i − NH) ∫0 ∫ ij ij i Basic references: C. -
Notes on Semiclassical Gravity
ANNALS OF PHYSICS 196, 296-M (1989) Notes on Semiclassical Gravity T. P. SINGH AND T. PADMANABHAN Theoretical Astrophvsics Group, Tata Institute of Fundamental Research, Horn; Bhabha Road, Bombay 400005, India Received March 31, 1989; revised July 6, 1989 In this paper we investigate the different possible ways of defining the semiclassical limit of quantum general relativity. We discuss the conditions under which the expectation value of the energy-momentum tensor can act as the source for a semiclassical, c-number, gravitational field. The basic issues can be understood from the study of the semiclassical limit of a toy model, consisting of two interacting particles, which mimics the essential properties of quan- tum general relativity. We define and study the WKB semiclassical approximation and the gaussian semiclassical approximation for this model. We develop rules for Iinding the back- reaction of the quantum mode 4 on the classical mode Q. We argue that the back-reaction can be found using the phase of the wave-function which describes the dynamics of 4. We find that this back-reaction is obtainable from the expectation value of the hamiltonian if the dis- persion in this phase can be neglected. These results on the back-reaction are generalised to the semiclassical limit of the Wheeler-Dewitt equation. We conclude that the back-reaction in semiclassical gravity is ( Tlk) only when the dispersion in the phase of the matter wavefunc- tional can be neglected. This conclusion is highlighted with a minisuperspace example of a massless scalar field in a Robertson-Walker universe. We use the semiclassical theory to show that the minisuperspace approximation in quantum cosmology is valid only if the production of gravitons is negligible. -
Introduction to General Relativity
INTRODUCTION TO GENERAL RELATIVITY Gerard 't Hooft Institute for Theoretical Physics Utrecht University and Spinoza Institute Postbox 80.195 3508 TD Utrecht, the Netherlands e-mail: [email protected] internet: http://www.phys.uu.nl/~thooft/ Version November 2010 1 Prologue General relativity is a beautiful scheme for describing the gravitational ¯eld and the equations it obeys. Nowadays this theory is often used as a prototype for other, more intricate constructions to describe forces between elementary particles or other branches of fundamental physics. This is why in an introduction to general relativity it is of importance to separate as clearly as possible the various ingredients that together give shape to this paradigm. After explaining the physical motivations we ¯rst introduce curved coordinates, then add to this the notion of an a±ne connection ¯eld and only as a later step add to that the metric ¯eld. One then sees clearly how space and time get more and more structure, until ¯nally all we have to do is deduce Einstein's ¯eld equations. These notes materialized when I was asked to present some lectures on General Rela- tivity. Small changes were made over the years. I decided to make them freely available on the web, via my home page. Some readers expressed their irritation over the fact that after 12 pages I switch notation: the i in the time components of vectors disappears, and the metric becomes the ¡ + + + metric. Why this \inconsistency" in the notation? There were two reasons for this. The transition is made where we proceed from special relativity to general relativity. -
Unitarity Condition on Quantum Fields in Semiclassical Gravity Abstract
KNUTH-26,March1995 Unitarity Condition on Quantum Fields in Semiclassical Gravity Sang Pyo Kim ∗ Department of Physics Kunsan National University Kunsan 573-701, Korea Abstract The condition for the unitarity of a quantum field is investigated in semiclas- sical gravity from the Wheeler-DeWitt equation. It is found that the quantum field preserves unitarity asymptotically in the Lorentzian universe, but does not preserve unitarity completely in the Euclidean universe. In particular we obtain a very simple matter field equation in the basis of the generalized invariant of the matter field Hamiltonian whose asymptotic solution is found explicitly. Published in Physics Letters A 205, 359 (1995) Unitarity of quantum field theory in curved space-time has been a problem long debated but sill unsolved. In particular the issue has become an impassioned altercation with the discovery of the Hawking radiation [1] from black hole in relation to the information loss problem. Recently there has been a series of active and intensive investigations of quantum ∗E-mail : [email protected] 1 effects of matter field through dilaton gravity and resumption of unitarity and information loss problem (for a good review and references see [2]). In this letter we approach the unitarity problem and investigate the condition for the unitarity of a quantum field from the point of view of semiclassical gravity based on the Wheeler-DeWitt equation [3]. By developing various methods [4–18] for semiclassical gravity and elaborating further the new asymptotic expansion method [19] for the Wheeler-DeWitt equation, we derive the quantum field theory for a matter field from the Wheeler-DeWittt equation for the gravity coupled to the matter field, which is equivalent to a gravitational field equation and a matrix equation for the matter field through a definition of cosmological time. -
Inflation Without Quantum Gravity
Inflation without quantum gravity Tommi Markkanen, Syksy R¨as¨anen and Pyry Wahlman University of Helsinki, Department of Physics and Helsinki Institute of Physics P.O. Box 64, FIN-00014 University of Helsinki, Finland E-mail: tommi dot markkanen at helsinki dot fi, syksy dot rasanen at iki dot fi, pyry dot wahlman at helsinki dot fi Abstract. It is sometimes argued that observation of tensor modes from inflation would provide the first evidence for quantum gravity. However, in the usual inflationary formalism, also the scalar modes involve quantised metric perturbations. We consider the issue in a semiclassical setup in which only matter is quantised, and spacetime is classical. We assume that the state collapses on a spacelike hypersurface, and find that the spectrum of scalar perturbations depends on the hypersurface. For reasonable choices, we can recover the usual inflationary predictions for scalar perturbations in minimally coupled single-field models. In models where non-minimal coupling to gravity is important and the field value is sub-Planckian, we do not get a nearly scale-invariant spectrum of scalar perturbations. As gravitational waves are only produced at second order, the tensor-to-scalar ratio is negligible. We conclude that detection of inflationary gravitational waves would indeed be needed to have observational evidence of quantisation of gravity. arXiv:1407.4691v2 [astro-ph.CO] 4 May 2015 Contents 1 Introduction 1 2 Semiclassical inflation 3 2.1 Action and equations of motion 3 2.2 From homogeneity and isotropy to perturbations 6 3 Matching across the collapse 7 3.1 Hypersurface of collapse 7 3.2 Inflation models 10 4 Conclusions 13 1 Introduction Inflation and the quantisation of gravity. -
Open Dissertation-Final.Pdf
The Pennsylvania State University The Graduate School The Eberly College of Science CORRELATIONS IN QUANTUM GRAVITY AND COSMOLOGY A Dissertation in Physics by Bekir Baytas © 2018 Bekir Baytas Submitted in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy August 2018 The dissertation of Bekir Baytas was reviewed and approved∗ by the following: Sarah Shandera Assistant Professor of Physics Dissertation Advisor, Chair of Committee Eugenio Bianchi Assistant Professor of Physics Martin Bojowald Professor of Physics Donghui Jeong Assistant Professor of Astronomy and Astrophysics Nitin Samarth Professor of Physics Head of the Department of Physics ∗Signatures are on file in the Graduate School. ii Abstract We study what kind of implications and inferences one can deduce by studying correlations which are realized in various physical systems. In particular, this thesis focuses on specific correlations in systems that are considered in quantum gravity (loop quantum gravity) and cosmology. In loop quantum gravity, a spin-network basis state, nodes of the graph describe un-entangled quantum regions of space, quantum polyhedra. We introduce Bell- network states and study correlations of quantum polyhedra in a dipole, a pentagram and a generic graph. We find that vector geometries, structures with neighboring polyhedra having adjacent faces glued back-to-back, arise from Bell-network states. The results present show clearly the role that entanglement plays in the gluing of neighboring quantum regions of space. We introduce a discrete quantum spin system in which canonical effective methods for background independent theories of quantum gravity can be tested with promising results. In particular, features of interacting dynamics are analyzed with an emphasis on homogeneous configurations and the dynamical building- up and stability of long-range correlations. -
"Eternal" Questions in the XX-Century Theoretical Physics V
Philosophical roots of the "eternal" questions in the XX-century theoretical physics V. Ihnatovych Department of Philosophy, National Technical University of Ukraine “Kyiv Polytechnic Institute”, Kyiv, Ukraine e-mail: [email protected] Abstract The evolution of theoretical physics in the XX century differs significantly from that in XVII-XIX centuries. While continuous progress is observed for theoretical physics in XVII-XIX centuries, modern physics contains many questions that have not been resolved despite many decades of discussion. Based upon the analysis of works by the founders of the XX-century physics, the conclusion is made that the roots of the "eternal" questions by the XX-century theoretical physics lie in the philosophy used by its founders. The conclusion is made about the need to use the ideas of philosophy that guided C. Huygens, I. Newton, W. Thomson (Lord Kelvin), J. K. Maxwell, and the other great physicists of the XVII-XIX centuries, in all areas of theoretical physics. 1. Classical Physics The history of theoretical physics begins in 1687 with the work “Mathematical Principles of Natural Philosophy” by Isaac Newton. Even today, this work is an example of what a full and consistent outline of the physical theory should be. It contains everything necessary for such an outline – definition of basic concepts, the complete list of underlying laws, presentation of methods of theoretical research, rigorous proofs. In the eighteenth century, such great physicists and mathematicians as Euler, D'Alembert, Lagrange, Laplace and others developed mechanics, hydrodynamics, acoustics and nebular mechanics on the basis of the ideas of Newton's “Principles”. -
The Universe Unveiled Given by Prof Carlo Contaldi
Friends of Imperial Theoretical Physics We are delighted to announce that the first FITP event of 2015 will be a talk entitled The Universe Unveiled given by Prof Carlo Contaldi. The event is free and open to all but please register by visiting the Eventbrite website via http://tinyurl.com/fitptalk2015. Date: 29th April 2015 Venue: Lecture Theatre 1, Blackett Laboratory, Physics Department, ICL Time: 7-8pm followed by a reception in the level 8 Common room Speaker: Professor Carlo Contaldi The Universe Unveiled The past 25 years have seen our understanding of the Universe we live in being revolutionised by a series of stunning observational campaigns and theoretical advances. We now know the composition, age, geometry and evolutionary history of the Universe to an astonishing degree of precision. A surprising aspect of this journey of discovery is that it has revealed some profound conundrums that challenge the most basic tenets of fundamental physics. We still do not understand the nature of 95% of the matter and energy that seems to fill the Universe, we still do not know why or how the Universe came into being, and we have yet to build a consistent "theory of everything" that can describe the evolution of the Universe during the first few instances after the Big Bang. In this lecture I will review what we know about the Universe today and discuss the exciting experimental and theoretical advances happening in cosmology, including the controversy surrounding last year's BICEP2 "discovery". Biography of the speaker: Professor Contaldi gained his PhD in theoretical physics in 2000 at Imperial College working on theories describing the formation of structures in the universe.