Florian Girelli 2. General construction of DSR 3. Exploring the physics of DSR 1. DSR: phenomenology of QG.

Slides:



Advertisements
Similar presentations
H6: Relativistic momentum and energy
Advertisements

Lecture 20 Relativistic Effects Chapter Outline Relativity of Time Time Dilation Length Contraction Relativistic Momentum and Addition of Velocities.
F. Debbasch (LERMA-ERGA Université Paris 6) and M. Bustamante, C. Chevalier, Y. Ollivier Statistical Physics and relativistic gravity ( )
Theories of gravity in 5D brane-world scenarios
General Relativity Physics Honours 2006 A/Prof. Geraint F. Lewis Rm 557, A29 Lecture Notes 9.
Dark Energy and Quantum Gravity Dark Energy and Quantum Gravity Enikő Regős Enikő Regős.
Massive Gravity and the Galileon Claudia de Rham Université de Genève Work with Gregory Gabadadze, Lavinia Heisenberg, David Pirtskhalava and Andrew Tolley.
Rainbow Gravity and the Very Early Universe Yi Ling Center for Gravity and Relativistic Astrophysics Nanchang University, China Nov. 4, Workshop.
Light Bending as a probe of Geometric Dark Energy modelsEDEN, Paris December 8,2005 Light Bending as a probe for Geometric Dark Energy Alessandro Gruppuso.
Covariant Formulation of the Generalized Lorentz Invariance and Modified Dispersion Relations Alex E. Bernardini Departamento de Física – UFSCAR Financial.
Relativistic effects High Energy Astrophysics 2009.
EPPT M2 INTRODUCTION TO RELATIVITY K Young, Physics Department, CUHK  The Chinese University of Hong Kong.
General Relativity Physics Honours 2008 A/Prof. Geraint F. Lewis Rm 557, A29 Lecture Notes 2.
Lecture 23 Models with Cosmological Constant ASTR 340 Fall 2006 Dennis Papadopoulos Chapter 11 Problems Due 12/5/06.
General Relativity Physics Honours 2007 A/Prof. Geraint F. Lewis Rm 557, A29 Lecture Notes 4.
The Ideas of Unified Theories of Physics Tareq Ahmed Mokhiemer PHYS441 Student.
Mohamed Anber HEP Bag Lunch April 1st With Lorenzo Sorbo
The Cosmological Constant and Technical Naturalness Sunny Itzhaki hep-th/ work to appear.
Physics 133: Extragalactic Astronomy ad Cosmology Lecture 4; January
Macroscopic Behaviours of Palatini Modified Gravity Theories [gr-qc] and [gr-qc] Baojiu Li, David F. Mota & Douglas J. Shaw Portsmouth,
Chapter 12 Gravitation. Theories of Gravity Newton’s Einstein’s.
How does the universe expand? What is expansion? Newtonian derivation of FRW-equations Problems with FRW: causality General Relativity derivation of FRW-
Classical Mechanics and Special Relativity with GA Suprit Singh.
Renormalization group scale-setting in astrophysical systems Silvije Domazet Ru đ er Bošković Institute,Zagreb Theoretical Physics Division th.
Kaluza-Klein gluon production at the LHC
M ultiverse and the Naturalness Problem Hikaru KAWAI 2012/ 12/ 4 at Osaka University.
Two Higgs doublets model in gauge-Higgs unification framework Yonsei University Jubin Park (SNUT)  Collaboration with Prof. We-Fu Chang,
Cascading gravity and de gravitation Claudia de Rham Perimeter Institute/McMaster Miami 2008 Dec, 18 th 2008.
MA4248 Weeks 1-3. Topics Coordinate Systems, Kinematics, Newton’s Laws, Inertial Mass, Force, Momentum, Energy, Harmonic Oscillations (Springs and Pendulums)
Relativistic Mass and Energy
Lecture 6 Momentum, Relativity, Energy and Civilization Chapter 3.8  3.15 Outline Linear Momentum Angular Momentum Relativity and Rest Energy Energy and.
String Theory Quantum Mechanics and Gravity: The start of a beautiful relationship? Cliff Burgess.
RELATIVITY.
Quantum Effects From Boundaries in de Sitter and anti-de Sitter spaces Aram Saharian Department of Physics, Yerevan State University, Armenia _________________________________________.
One Dimensional Kinematics: Problem Solving Kinematics in Two-Dimensions: Law of Addition of Velocities Projectile Motion 8.01 W02D1.
Giuseppe De Risi M. Cavaglià, G.D., M. Gasperini, Phys. Lett. B 610:9-17, hep-th/ QG05, Sept
General Relativity Physics Honours 2005 Dr Geraint F. Lewis Rm 557, A29
Special Relativity The Failure of Galilean Transformations
Particle Interactions with Modified Dispersion Relations Yi Ling (凌意) IHEP,CAS & Nanchang University 2012 两岸粒子物理与宇宙学研讨会, 重庆,05/09/2012.
General Relativity Physics Honours 2009
Influence of dark energy on gravitational lensing Kabita Sarkar 1, Arunava Bhadra 2 1 Salesian College, Siliguri Campus, India High Energy Cosmic.
General Relativity Physics Honours 2008 A/Prof. Geraint F. Lewis Rm 560, A29 Lecture Notes 9.
Possible Enhancement of noncommutative EFFECTS IN gravity Objective Look for consequences of gravity on noncommutative (NC) space-time Chamseddine In particular,
Emergence of space, general relativity and gauge theory from tensor models Naoki Sasakura Yukawa Institute for Theoretical Physics.
Space-time Invariance and Quantum Gravity By Dr. Harold WilliamsDr. Harold Williams of Montgomery College PlanetariumMontgomeryCollegePlanetarium.
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang.
Gravitation in 3D Spacetime John R. Laubenstein IWPD Research Center Naperville, Illinois APS April Meeting Denver, Colorado.
SOME REFLECTIONS ON A POSSIBLE HOLOGRAPHIC DESCRIPTION OF TIME CHAPTER IN PROGRESS FOR MY FORTHCOMING BOOK “THE EMERGENCE OF SPACETIME IN STRING THEORY”
Chapter 36 The Special Theory of Relativity (Special Relativity Principle)
The force law in relativity Consider an object that is accelerated by a constant force F, for example a space traveler in a rocket ship. Newton’s force.
Chapter 1. The principle of relativity Section 1. Velocity of propagation of interaction.
By: Jennifer Doran. What was Known in 1900 Newton’s laws of motion Maxwell’s laws of electromagnetism.
Celestial Mechanics IV Central orbits Force from shape, shape from force General relativity correction.
University of Oslo & Caltech
“Applied” String Theory Pinaki Banerjee The Institute of Mathematical Sciences, Chennai Department of Physics, Visva Bharati 12 th July, 2013.
Anisotropic Mechanics J.M. Romero, V. Cuesta, J.A. Garcia, and J. D. Vergara Instituto de Ciencias Nucleares, UNAM, Mexico.
String Theory: A Short Introduction By Seamus O’Dunn Monday, October 22, 2012.
Relativistic mechanics
Dept.of Physics & Astrophysics
Florian Girelli: I decided to study the fundamental nature of space-time when finishing high-school. My university/research cursus: Master of Mathematics.
Unruh’s Effect Savan Kharel.
Institut d’Astrophysique de Paris
Ariel Edery Bishop’s University
Derek Kan Khalid Mansour Ian Nickles
Relativistic Classical Mechanics
Translations in Relative Locality
A Swampland Update Cumrun Vafa Harvard University PASCOS 2019
Expressing n dimensions as n-1
2.11: Relativistic Momentum Because physicists believe that the conservation of momentum is fundamental, we begin by considering collisions where.
Presentation transcript:

Florian Girelli 2. General construction of DSR 3. Exploring the physics of DSR 1. DSR: phenomenology of QG

QUANTUM GRAVITY String Theory Causal Sets Loop Quantum Gravity

Philosophy behind DSR  Instead of deriving a semi classical limit of the Quantum Gravity Theory, derive an effective theory from a well known theory: Special Relativity.  To this aim one introduces characteristic scales of Quantum Gravity:  One has to modify the symmetries in order to accommodate these new constants. Special Relativity is the first example of such process (cf talk by Chryssomalis earlier).  Physics of DSR should be different than relativistic physics, as much as relativistic physics is different than newtonian physics.  The resulting theory should describe a low energy phenomenology, directly testable mainly in astrophysical context (gamma ray, cosmic rays).

Special Relativity as an inspiration  Let us take the Schwarzschild ratio:  For spherical bodies (of radius L ) of rest mass M, we always need: We would like to incorporate this “new” universal constant in the relativistic context: incorporate a feature of gravity, without having gravity.  This is remnant of Special Relativity: we have a maximum length per unit of time.

Let Special Relativity guide us!  To implement a maximum speed in Special Relativity we modify the space of speeds into an hyperboloid.  The addition of the speeds is then modified! Indeed we want that the sum of speeds to be still smaller than the speed of light.

 On the configuration space, we have the notion of space-time that appears.  We have the relativistic speed such that  Physical objects are given in terms of linear representations of the Poincare group ISO(3,1).

Let’s do the same with momentum now!  We are going to implement a maximum rest mass, we choose the Planck mass,.  We define a DSR momentum, The relativistic momentum is now defined as We have therefore now a momentum which rest mass is bounded by the Planck mass.

 Addition of momenta is on the de Sitter space: the rest mass is always bounded. If we define the addition in this way, we run in the soccer ball problem: the cutoff is not renormalized.  To recover additive quantities one needs to get to the Poincare-de Sitter group ISO(4,1).  Addition of the pentamomenta naturally implies a renormalization of the maximum mass: maximum mass is the 5 dimensional mass.  There exists other coordinate systems: physical interpretation is different, as a different quantity is bounded. Bicrossproduct basis: 3-momentum is bounded, with associative addition of relativistic momenta. Bicrossproduct basis: 3-momentum is bounded, with associative addition of relativistic momenta. Magueijo-Smolin basis: Energy is bounded, with addition of momenta highly non associative.

What about space-time?? There exists different approaches to reconstruct space time: 1.5d approach: space-time-mass (already introduced by Wesson) and its variants. 2.4d approach: 1.Coordinates as tangent vectors (Snyder’s approach, but also in the Minkowski space.) 2.Rainbow metric (Magueijo’s approach). This approach can be seen as 4d projection of the 5d construction.

Physics is about dynamics  By specifying some dynamics we should be able to eliminate some possibilities, in particular make also the distinction between 4d and 5d.  4d case: –Inertial observer: Casimir of the (deformed) symmetry: –Uniformly accelerated observer (work in progress): A massive body seems to reach the speed of light (in the Magueijo-Smolin setting)….

 5d case (work in progress):  The new physics is hidden in the fifth dimension sector, but very tiny physics This has to be deepened…

Conclusions  I recalled the general construction for DSR, and showed the parallel with Special Relativity.  I mentioned the main problems of DSR: the many bodies state (soccer ball problem) and the interpretation of dynamics.  I argued that a 5d approach should provide a better angle of attack to make a consistent theoretical framework.  DSR is extremely interesting: –Very close to Special Relativity –It can be related to the Space-Time-Mass introduced by Wesson: A non compactified Kaluza-Klein theory, where the extra dimension is the “mass”. This theory has been developed in the astrophysical and cosmological context and is still consistent with observations.  Most exciting: the field theory approach hasn’t been developed yet –It should provide a cutoff consistent with symmetries: natural regularization –It must be related to Percacci’s approach –Then potential relation with Randall-Sundrum model.