Quantum Gravity Why is it so Difficult? Craig Dowell February 24, 2006.

Slides:



Advertisements
Similar presentations
Rae §2.1, B&J §3.1, B&M § An equation for the matter waves: the time-dependent Schrődinger equation*** Classical wave equation (in one dimension):
Advertisements

From Quantum Mechanics to Lagrangian Densities
Quantum One: Lecture 6. The Initial Value Problem for Free Particles, and the Emergence of Fourier Transforms.
The electromagnetic (EM) field serves as a model for particle fields
Lecture 2. A Day of Principles The principle of virtual work d’Alembert’s principle Hamilton’s principle 1 (with an example that applies ‘em all at the.
Quantum One: Lecture 5a. Normalization Conditions for Free Particle Eigenstates.
1 Chapter 40 Quantum Mechanics April 6,8 Wave functions and Schrödinger equation 40.1 Wave functions and the one-dimensional Schrödinger equation Quantum.
One assumes: (1) energy, E  (- ℏ /i)  /  t (2) momentum, P  ( ℏ /i)  (3) particle probability density,  (r,t)  = i  /  x + j  /  y + k  / 
Wavefunction Quantum mechanics acknowledges the wave-particle duality of matter by supposing that, rather than traveling along a definite path, a particle.
The electromagnetic (EM) field serves as a model for particle fields  = charge density, J = current density.
Given the Uncertainty Principle, how do you write an equation of motion for a particle? First, remember that a particle is only a particle sort of, and.
2. Solving Schrödinger’s Equation Superposition Given a few solutions of Schrödinger’s equation, we can make more of them Let  1 and  2 be two solutions.
4. The Postulates of Quantum Mechanics 4A. Revisiting Representations
The Harmonic Oscillator
Ch 9 pages ; Lecture 21 – Schrodinger’s equation.
PHYS 3313 – Section 001 Lecture #17
Anharmonic Oscillator Derivation of Second Order Susceptibilities
Vibrational Spectroscopy
The World Particle content. Interactions Schrodinger Wave Equation He started with the energy-momentum relation for a particle he made the quantum.
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.
The World Particle content All the particles are spin ½ fermions!
What do we know about the Standard Model? Sally Dawson Lecture 2 SLAC Summer Institute.
Operators A function is something that turns numbers into numbers An operator is something that turns functions into functions Example: The derivative.
Absorption and Emission of Radiation:
Ch ; Lecture 26 – Quantum description of absorption.
Physics 2170 – Spring The Schrödinger equation Next homework assignment is available I will be giving a.
Wednesday, Mar. 5, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #13 Wednesday, Mar. 5, 2003 Dr. Jae Yu Local Gauge Invariance and Introduction.
Wednesday, Oct. 17, 2012PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #13 Wednesday, Oct. 17, 2012 Dr. Jaehoon Yu Properties.
Lecture 15 Solving the time dependent Schrödinger equation
The Quantum Theory of Atoms and Molecules The Schrödinger equation and how to use wavefunctions Dr Grant Ritchie.
Gerard ’t Hooft, quant-ph/ Erice, September 6, 2006 Utrecht University 1.
Simple Harmonic Oscillator (SHO) Quantum Physics II Recommended Reading: Harris: chapter 4 section 8.
Characteristic vibrations of the field. LL2 section 52.
Quantum Mechanical Cross Sections In a practical scattering experiment the observables we have on hand are momenta, spins, masses, etc.. We do not directly.
One particle states: Wave Packets States. Heisenberg Picture.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #4.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #2.
Back to basics The three fundamental units G, c, ћ are sufficient to describe all the quantities that appear in physics. They are.
Physics Lecture 11 3/2/ Andrew Brandt Monday March 2, 2009 Dr. Andrew Brandt 1.Quantum Mechanics 2.Schrodinger’s Equation 3.Wave Function.
LECTURE 17 THE PARTICLE IN A BOX PHYSICS 420 SPRING 2006 Dennis Papadopoulos.
The Importance of the TeV Scale Sally Dawson Lecture 3 FNAL LHC Workshop, 2006.
MODULE 13 Time-independent Perturbation Theory Let us suppose that we have a system of interest for which the Schrödinger equation is We know that we can.
5. The Harmonic Oscillator Consider a general problem in 1D Particles tend to be near their minimum Taylor expand V(x) near its minimum Recall V’(x 0 )
An equation for matter waves Seem to need an equation that involves the first derivative in time, but the second derivative in space As before try solution.
Quantum One.
The Quantum Theory of Atoms and Molecules
Quantum Field Theory (PH-537) M.Sc Physics 4th Semester
Chapter 40 Quantum Mechanics
Quantum Mechanics for Applied Physics
Schrodinger wave equation
Quantum Mechanics.
Chapter V Interacting Fields Lecture 1 Books Recommended:
Quantum Mechanics for Scientists and Engineers
CHAPTER 5 The Schrodinger Eqn.
Derivation of Electro-Weak Unification and Final Form of Standard Model with QCD and Gluons  1W1+  2W2 +  3W3.
CHAPTER 5 The Schrodinger Eqn.
Quantum One.
4. The Postulates of Quantum Mechanics 4A. Revisiting Representations
Quantum One.
2. Solving Schrödinger’s Equation
Quantum One.
Quantum Two.
The World Particle content.
Chapter V Interacting Fields Lecture 7 Books Recommended:
Chapter 40 Quantum Mechanics
Quantum Mechanics.
Adaptive Perturbation Theory: QM and Field Theory
Adnan Bashir, UMSNH, Mexico
Renormalization and the renormalization group
It means anything not quadratic in fields and derivatives.
Presentation transcript:

Quantum Gravity Why is it so Difficult? Craig Dowell February 24, 2006

Quantum Gravity: Why so Difficult? Why Quantum Gravity? Two Great Theories Revolutionized Physics Quantum Mechanics (verified to great precision) General Relativity (verified to great precision) Three of Four Fundamental Forces are described by QFT Gravity is the Odd Theory Out Would be Nice to Know What Happens When Quantum and Gravitational Effects are Both Large?

Quantum Gravity: Why so Difficult? Two Paths to a Quantum Theory of Gravity Start with General Relativity and Rewrite Quantum Field Theory Loop Quantum Gravity Start with Quantum Field Theory and Reformulate General Relativity Quantum Gravity String Theory I will focus on Quantum Gravity Today Specifically on Why it is Difficult to Make a Working Theory

Quantum Gravity: Why so Difficult? The Problem Infinities when Calculating Probabilities Basically, it all Translates Into a Normalization Problem, i.e. Where Does the Problem Come From? Let’s Start Slowly From the Beginning

Quantum Gravity: Why so Difficult? Normalization The Statistical Interpretation of Quantum Mechanics Says that, Represents the Probability of Finding the Particle at point x at time t. The Sum of the Probabilities of the Particle being in all Possible Places must be Unity Finding the Coefficient N so that this is True is Called Normalizing the Wavefunction

Quantum Gravity: Why so Difficult? Time Independent Perturbation Theory You Take a Hamiltonian Corresponding to an Exact Solution to the Schrodinger Equation and Perturb It. Then you Expand in Terms of Power Series and Cutoff at some order. But You Originally Normalized for the Solved Wavefunction. You Have to Pick a New N – You have to Renormalize

Quantum Gravity: Why so Difficult? Time Independent Perturbation Theory II What if One of the Terms is Infinite? The Integral Diverges. There is no N That Can Fix the Problem The New Wavefunction is Nonrenormalizable. Calculations Using the Wavefunction Would Produce Infinite Probabilities, Which is Nonsense. We’ll See That a Similar Problem Causes the Infinities in Quantum Gravity

Quantum Gravity: Why so Difficult? What is Quantum Field Theory? Recall that Maxwell’s Equations in Free Space Imply the Existence of Electromagnetic Waves Imagine a Rectangular Resonant Cavity with a Standing Wave in the z direction. The E and B Fields Could be Make a Hamiltonian from the Energy Density (in 1-D)

Quantum Gravity: Why so Difficult? What is Quantum Field Theory? (II) The Resulting Hamiltonian looks like the Hamiltonian for a Harmonic Oscillator. A Single Mode of an Electromagnetic Field in a One-Dimensional Cavity is a Harmonic Oscillator Recall Harmonic Oscillators From Quantum Mechanics Call the raising operator and use it as a photon creation operator Call the lowering operator and use it as a photon annihilation operator. The Fourier Components of the Electromagnetic Field are Quantized as Harmonic Oscillators

Quantum Gravity: Why so Difficult? Quantum Theory of Your Mattress Spring Imagine the Collection of Harmonic Oscillators as Springs. Vertices (Blue Rings) are Point Masses If You Strike the Mattress, Waves Propagate. If You Strike in Two Places, Waves Superpose

Quantum Gravity: Why so Difficult? Quantum Theory of Your Mattress Spring (II) We Want to Model Interacting Particles, Not Particles that Move Through Each Other. Harmonic Oscillators Do Not Allow for Particle Interactions Anharmonic Oscillators Allow for Particle Interactions. Anharmonic Oscillators Cannot Be Solved Exactly Must Resort to Approximation. Think Perturbation Theory. That’s Why We Looked at Time Independent Perturbation Theory The Correction Terms are Where Those Infinities Will Come In.

Quantum Gravity: Why so Difficult? Some More Quantum Mechanics Recall the Schrodinger Equation It Was Solved by Separation of Variables and We Found that the Time Dependence Was This Unitary Operator Governs the Amplitude to go from One Place to Another Now a Feynman Story

Quantum Gravity: Why so Difficult? The Smart-Aleck High-School Physics Student Double Slit Experiment. Amplitude is sum of probabilities of both paths What Happens if you Drill Two More Holes Sum of Probabilities Includes New Holes What Happens if you Add Another Screen Sum of Probabilities Includes Paths Through Holes in New Screen What if You Drill an Infinite Number of Holes in The Screens So That They are No Longer There You discover the Feynman Sum over Paths Approach to Quantum Field Theory.

Quantum Gravity: Why so Difficult? The Path Integral Dirac Derived the Path Integral Representation of the Feynman Sum over Paths Statement. It Turns Out That if You Write the Hamiltonian for the Harmonic Oscillator as H, you get You Can See That the Lagrangian of the Harmonic Oscillator Pops Out

Quantum Gravity: Why so Difficult? The Path Integral (II) Sometimes this is written in terms of the action S. It’s Not Too Much of a Stretch Now to Add an Anharmonicity Term The Indicates We are Integrating over Spacetime, and the Indicates We are Talking about Fields. The is the Perturbation Causing Anharmonicity and Represents a Force (think of pushing on the mattress).

Quantum Gravity: Why so Difficult? Summary Quantum Field Theory is No Big Deal. All You Have to do is to Evaluate the Path Integral.

Quantum Gravity: Why so Difficult? Summary Quantum Field Theory is No Big Deal. All You Have to do is to Evaluate the Path Integral. Oh, Except for One Thing …

Quantum Gravity: Why so Difficult? Summary Quantum Field Theory is No Big Deal. All You Have to do is to Evaluate the Path Integral. Oh, Except for One Thing … The Integral is Impossible to do

Quantum Gravity: Why so Difficult? Feynman to the Rescue Came up With a Process to Approximate the Solution by Series Solution in Called the Coupling Constant. To Keep Track of the Terms in the Expansion, We Draw Little Diagrams. Each Part of the Diagram Corresponds to a Rule. If You Walk Through the Diagram and Apply the Rules, You Can Write Down a Solution to the Path Integral Feynman Diagrams are a Convenient Way of Representing a Double Series Expansion in and

Quantum Gravity: Why so Difficult? Storm Clouds It Turns That if you Follow the Rules That Describe a Meson-Meson Scattering Event, the Correction to the Amplitude Diverges. It has the Form This Logarithmic Divergence Happens at Large k (momentum) – So it is Called an Ultraviolet Divergence. It Happens Whenever There is a Loop in a Feynman Diagram. If the Correction Diverges, the Amplitude Diverges and we Calculate an Infinite Probability – Nonsense. This is How Those Infinities Happen.

Quantum Gravity: Why so Difficult? All Feynman Diagrams with Loops Generate Terms Which Diverge! A Way Out Was Found The Process Involves Two Phases Regularization Renormalization

Quantum Gravity: Why so Difficult? Regularization We Have Found Integrals of the Form Which Diverge at Large k Why Not Integrate Up to a Large, but Not Infinite Momentum Parameterized by This is Called Momentum Cutoff Justification: We Decide That There is No Reason Our Theory Must be Valid to Arbitrarily Large Energies

Quantum Gravity: Why so Difficult? Regularization (II) The General Solution to the Integral is In the Limit, C Vanishes, B is Independent of and A diverges We Have Separated the Integral Into a Piece That is Infinite and a Piece That is Finite What If We Could Find a Way to Get Rid of the Infinite Part – Sweep it Under the Rug There is a Way Called Renormalization

Quantum Gravity: Why so Difficult? Renormalization We Have a Coupling Constant and a Cutoff What Do These Greek Letters Mean The Coupling Constant is a Real Measurable Value The Coupling Constant in Electrodynamics is That Shouldn’t Change Depending on the Arbitrary Cutoff we Choose – Who Decides What the Cutoff is and Why So if we Change Then Must Change to Compensate This Means that in the Real World, There is a Physical Coupling Constant and is Actually a Function of Let’s Look at a Real Example

Quantum Gravity: Why so Difficult? Renormalization (II) Warning, Lots of Equations Coming … A Theoretical Meson-Meson Scattering Amplitude Correction of Order is, After Integrating to a Cutoff To Make Our Lives Easier, We Define Where s, t and u are Momenta From the Feynman Diagram

Quantum Gravity: Why so Difficult? Renormalization (III) According to the Theory, If Someone Was to Go and Actually Physically Measure This Event, She Would Measure a Coupling Constant Predicted By Again, To Make Our Lives Easier, Define

Quantum Gravity: Why so Difficult? Renormalization (IV) If the Measurement is Done, We Predict Now Solve for We also Expect So, When We Say We Mean

Quantum Gravity: Why so Difficult? Renormalization (V) We Originally Predicted But We Really Meant That So, Combining the Two, What We Really Should Have Written is But Notice that

Quantum Gravity: Why so Difficult? Renormalization (VI) What Was So Did You See It? My Hands Never Left My Arms! The Cutoff is Gone into a Puff of Logic

Quantum Gravity: Why so Difficult? Renormalization (VII) Zee Says, We started out with two unphysical quantities and their unphysicalness sort of cancelled each other out. Blechman Says, Before you label this as ridiculous, realize that QED has used renormalization all the time, and its results have been tested to as many as fourteen decimal places. That is the best known confirmation of any theory of physics.

Quantum Gravity: Why so Difficult? Pause My Presentation is About Quantum Gravity We Needed to Understand Some Quantum Field Theory Before We Could Understand Why Gravity Didn’t Fit Now, on to Quantum Gravity

Quantum Gravity: Why so Difficult? In General Relativity Particles Move along Paths Which Extremize Proper Time Possible Paths are Described by the Action The Conditions for an Extremum of the Action are Lagrange’s Equations Particles Follow Geodesics Which Satisfy Lagrange’s Equations, So The Lagrangian is For a Spacetime With Metric

Quantum Gravity: Why so Difficult? How Would One do Quantum Gravity? Start with Einstein-Hilbert Action Extremize the Proper Time to find the Lagrangian Put the Lagrangian into the Feynman Path Integral Develop Feynman Rules Evaluate the Path Integral Regularize Renormalize Go to Disneyland

Quantum Gravity: Why so Difficult? Don’t Buy the Tickets Quite Yet Since the Action is in an Exponential, It Must be Dimensionless. Recall Notice That if Each Piece of the Lagrangian has Dimension 4 Then Has Dimension [1] Has Dimension [1] and Has Dimension [0] The Coupling Constant is Dimensionless

Quantum Gravity: Why so Difficult? Don’t Buy the Tickets Quite Yet (II) Remember We Did the Trick Where We Equated and to Renormalize That Was Equating to (the coupling constant of the electromagnetic field) Which is Dimensionless The Gravitational Coupling Constant is Dimensionful Then Has Dimension When We Try to Do the Equivalence Trick in the Series Expansion

Quantum Gravity: Why so Difficult? Don’t Buy the Tickets Quite Yet (III) What Does it Mean to Have an Infinite Series with Terms of Increasing Dimension? If You “Cutoff” the Series, You Can Apparently Fiddle with the Resulting Equations to Get Something With a Physical Meaning But You Cannot Renormalize Quantum Gravity is a Nonrenormalizable Theory You Cannot Get Rid of the Infinities in Interactions that Have Loops in The Feynman Diagrams

Quantum Gravity: Why so Difficult? Don’t Buy the Tickets Quite Yet (IV) Think About an Two Particles Interacting Gravitationally Quel Horreur! A Loop. Infinities. Nonsense.

Quantum Gravity: Yes It’s Difficult. Quantum Gravity is a Nonrenormalizable Theory That Blows up on Loops Gravitational Interactions are Full of Loops Zee Says, “Nonrenormalizable theories evoke fear and loathing in theoretical physicists.” I’ll That to Mean Difficult. Quantum Gravity is Difficult and Now We Know Why