Gerard ’t Hooft ENS Paris, October 2008 Utrecht University What is an A scientific day in memory of Philippe MEYER (1925 - 2007)

Slides:



Advertisements
Similar presentations
Gerard t Hooft Spinoza Institute, Utrecht University Utrecht University and.
Advertisements

Gerard t Hooft VSV `Leonardo da Vinci Symposium, TU Delft, March 16, 2007 Utrecht University.
The search for the God Particle
Quantum Theory The worst scientific theory of all time Dr Mark J Hadley Dept of Physics.
1 The Feasibility of Testing LHVTs in High Energy Physics 李军利 中国科学院 研究生院 桂林 In corporation with 乔从丰 教授 Phys.Rev. D74,076003, (2006)
1 quantum teleportation David Riethmiller 28 May 2007.
Zeeya Merali Is Science Compatible with Our Desire for Freedom? Barcelona meeting May 2010.
Theory of Everything Is there an end to Physics?.
Gerard ’t Hooft Dublin November 13, 2007 Utrecht University on.
Big Bang …..was actually very small and quiet. Atoms are mostly empty space.
and Stockholm, August 27, 2004 Gerard ’t Hooft Utrecht University The Nature of.
Gerard ’t Hooft Tilburg, Keynote Address Utrecht University the.
PHYS Quantum Mechanics “the dreams stuff is made of” PHYS Quantum Mechanics “the dreams stuff is made of” Dr Jon Billowes Nuclear Physics Group.
Dr Mark Hadley Parity Violation: The Biggest Scientific Blunder of the 20th Century?
T. K. Ng (HKUST) The Quantum Universe Modern picture of space-time, matter & forces What is reality in relatively and QM? (Twin paradox and Schrodinger.
Gerard ’t Hooft Spinoza Institute Utrecht University CMI, Chennai, 20 November 2009 arXiv:
Or Can all laws of nature be reduced to one single system?
Gerard ’t Hooft Utrecht April 15, 2008 Utrecht University.
Utrecht University Gerard ’t Hooft Gell-Mann Colloquium Singapore, February 24, 2010.
Dr Mark Hadley A Gravitational Explanation for Quantum Theory & non-time-orientable manifolds.
The Ideas of Unified Theories of Physics Tareq Ahmed Mokhiemer PHYS441 Student.
Welcome to GT5 Wormholes Time machines and Energy conditions Chairperson Dr. Mark Hadley MG11 Berlin.
PHYS Quantum Mechanics PHYS Quantum Mechanics Dr Gavin Smith Nuclear Physics Group These slides at:
PHYS Quantum Mechanics PHYS Quantum Mechanics Dr Jon Billowes Nuclear Physics Group (Schuster Building, room 4.10)
Gerard ’t Hooft Utrecht University and Mystery. Theme: - Nature is more beautiful than we think - Nature is smarter than we are The landscape around 1965:
Gerard ’t Hooft Santiago de Compostela December Utrecht University Can be at the Planck scale?
Gerard ’t Hooft Chennai, November 17, 2009 Utrecht University.
Einstein, String Theory, and the Future Jonathan Feng University of California, Irvine Einstein: A Century of Relativity Skirball Cultural Center, Los.
Fermions and non-commuting observables from classical probabilities.
4. The Postulates of Quantum Mechanics 4A. Revisiting Representations
CERN 22nd European School
Quantum Mechanics and General Relativity Astronomy 315 Professor Lee Carkner Special Lecture.
Galileo Galilei Colloquium, Pisa, March 3, 2006 Gerard ’t Hooft Utrecht University.
Niels Martens DPhil Candidate Philosophy of Physics Oxford University Why Philosophy of Physics is Awesome!
Why Philosophy of Physics is Awesome!
Gerard ’t Hooft CERN Colloquium Genève, January 11, 2007 Utrecht University Will there be hints from LHC ?
Space-time in the new millennium
Utrecht University Gerard ’t Hooft CERN Black Hole Institute.
Monday, Apr. 2, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #12, 13, 14 Monday, Apr. 2, 2007 Dr. Jae Yu 1.Local Gauge Invariance 2.U(1) Gauge.
Strings: Theory of Everything, Something, or Nothing? Robert N. Oerter.
Chapter 26 Relativity. General Physics Relativity II Sections 5–7.
S.MORRIS Bill Nye the Science Guy 0vu7cU&feature=related 0vu7cU&feature=related.
1 Are Black Holes Elementary Particles? Y.K. Ha Temple University years since Solvay 1933.
SEVEN DEADLY QUANTUM SINS
By Ryan Deetscreek and Greg Goettner
Einstein’s elusive waves
Intro to Cosmology! OR What is our Universe?. The Latest High Resolution Image of the Cosmic Microwave Background Radiation Low Energy RegionHigh Energy.
Quantum mechanical phenomena. The study between quanta and elementary particles. Quanta – an indivisible entity of a quantity that has the same value.
Gerard ’t Hooft, quant-ph/ Erice, September 6, 2006 Utrecht University 1.
Physics 2170 – Spring Some interesting aspects of quantum mechanics The last homework is due at 12:50pm.
Anthropology Series In the Beginning How did the Universe begin? Don’t know!
STANDARD MODEL class of “High Energy Physics Phenomenology” Mikhail Yurov Kyungpook National University November 15 th.
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #2.
The EPR Paradox, Bell’s inequalities, and its significance By: Miles H. Taylor.
Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004.
Announcements Grades for third exam are now available on WebCT Observing this week and next week counts on the third exam. Please print out the observing.
Bell’s Inequality.
Wednesday, Mar. 26, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #18 Monday, Mar. 26, 2003 Dr. Jae Yu Mass Terms in Lagrangians Spontaneous.
Cosmological Bell Inequalities Juan Maldacena AndyFest 2015 Warping the Universe: A celebration of the Science of Andrew Strominger.
Chapter 3 Postulates of Quantum Mechanics. Questions QM answers 1) How is the state of a system described mathematically? (In CM – via generalized coordinates.
Phy107 Fall From Last Time… Today Superposition of wave functions Indistinguishability Electron spin: a new quantum effect The Hydrogen atom and.
Macroscopic Quantum Geometry Craig Hogan University of Chicago and Fermilab.
DPG Conference, Hamburg
 All elementary particles in physics are classified as either fermions or bosons. Quantum physics demonstrates the particles may have an intrinsic non-zero.
Entangled Electrons.
Derek Kan Khalid Mansour Ian Nickles
Quantum mechanics from classical statistics
Quantum computation with classical bits
Propagation and Antennas
Presentation transcript:

Gerard ’t Hooft ENS Paris, October 2008 Utrecht University What is an A scientific day in memory of Philippe MEYER ( )

Particles in experiments Elementary vs Composite Unstable particles Pole in propagator Dressed and bare particles Particles in GR Particles at Horizons Gravitons The disputes about QM Ontological objects Protons, Photons and Phonons

Particles in experiments

Elementary vs Composite In Effective Quantum Field Theory, this distinction gradually disappears. Particles are elementary at one scale, composite at another. Use Ren. Group.

Is a black hole a composite particle ? Is a black hole a particle ? Is a particle a black hole ? Is technicolor a viable theory ? The Higgs as a shifted particle:

Unstable particles

Dressed and Bare Particles xx xx x x xx x

General Relativity: Particles in curved space-time

Particles and horizons, the hybrid picture

Is the graviton an elementary particle? Gauge dependence: not a problem, as in Yang-Mills... Is graviton distinct from matter ? gravity – matter unification... In “crystalline gravity”, space-time is a crystal where “defects” play the role of matter and gravitons. gravitons are as photons.

A particle is an energy quantum. Can this yet be a tangible, “ontological”, physical object? This leads to the disputes concerning the interpretation of quantum mechanics.

The Bohr – Einstein dispute. Today’s historians of science contend that the dispute was settled in favour of Niels Bohr: Quantum Mechanics is non-deterministic. J.S. Bell is said to have settled the issue with the Bell Inequalities.

A new variety of the same idea: the Conway – Kochen Free Will Theorem Consider two entangled massive spin 1 particles, with total spin S = 0 :

In case of spin 2 : 1 1 0

The 4 cubes of Conway & Kochen It is impossible to attach 0’s and 1’s to all axes at the positions of the dots, such that all orthogonal triples of axes have exactly the (1,1,0) combination.

Source 1 2 Conclude: Free Will Theorem: If observers on the two different sites have the free will to choose which axes to pick, the spin values of the two particles cannot be pre-determined. No “hidden variables ”

This proves (once again) that particles are NOT accompanied by “hidden variables” that dictate: < if you choose this axis, then you measure this value for the spin > But it does not disprove hidden variable models of a more delicate nature: There could be field variables at ultra short distance scales, that evolve deterministically, while non-commuting quantum operators are still needed to handle the statistics at intermediate scales.

In such theories, what we call elementary particles today, are not exactly eigenstates of the “ontological” observables (beables). They are eigenstates of non-commuting operators, even though the evolution of the system may be deterministic: a large class of commuting operators evolve into operators that still commute with them – the beables.

Compare: protons photons phonons

An elementary particle is a calculational unit. Its appearance may vary, depending on cicumstances. Under some conditions it may appear to be very real, being something that can be detected in a piece of apparatus. But in other cases its ontological status is much more vague.