Zwiebach text assumed

Hi everyone,

I believe there has been sufficient time since the first day of class for everyone to get hold of a copy of the Zwiebach textbook by now. I will therefore be assuming, from now on, that everyone does have a copy of Zwiebach.

Anyone for whom this presents undue hardship should let me know privately. Email will be best for a few more days yet – I am still recovering from a cough/throat bug.

Cheers,

Prof.Peet.

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Lecture 30 Jan

Focus for today: the light front gauge:

  1. light-front (LF) coordinates X^+, X^- ;
  2. noncovariant physical gauges, such as LF gauge, for handling string worldsheet reparametrization invariance;
  3. consequences for string equations of motion, boundary conditions, conserved momenta, and constraints;
  4. open string mode expansion, and the special case of X^- in LF gauge;
  5. Virasoro modes;
  6. the classical string mass formula.

The relevant chapter of Zwiebach (Z) is chapter (ch.)9.

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Lecture 25 Jan

This lecture, on Worldsheet symmetry currents and conserved quantum numbers, is related to Chapter Eight of Zwiebach.

Here are my lecture notes

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Homework Due Dates

Hi all,

Homeworks will be due on Fridays, at the start of lecture (with a five minute grace period, that means due before 11:15am).

Homeworks will be posted in their entirety by two weeks before the due date, although initial problems may appear before then.  For example, while two questions are already posted by today for Homework 1, the remaining questions will appear by Friday.

Cheers,

Prof. Peet.

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Grading Calendar

Here is the (tentative) Grading Calendar Schedule of when homework assignments are given out and when they are due.

Please note the grading weighting proposed:-

  • 10% in-class participation;
  • 50% homeworks (5×10%);
  • 40% final oral presentation.

Note: on all assessment instruments, answers will be graded on physical accuracy and quality of explanation.

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Topic schedule pre-break

20080109: organizational meeting [Zwiebach Chapter 1]

20080111: modern high-energy theory, unification, and physical motivations for string theory; classical and quantum physics of relativistic point particles; [Zwiebach Chapters 2,3,5]

20080116: classical non-relativistic string theory; classical relativistic string theory and the Nambu-Goto action [Zwiebach Chapters 4,6]

20080118: reparametrization invariance; relativistic string equations of motion; consistent boundary conditions (i) Free-Endpoint (ii) Dirichlet, and D-branes; the Static Gauge; how open string endpoints move [Zwiebach Chapter 6]

20080123: reparametrization invariance and choosing worldsheet coordinates; worldsheet wave equation and constraints and their physical interpretation; general open string motion and the specific case of the rigid rotator [Zwiebach Chapter 7]

20080125: worldsheet symmetry currents; Lorentz symmetry and conserved quantum numbers [Zwiebach Chapter 8]

20080130: Light-front gauge; relativistic string dynamics in LF gauge and the constraint equations; Virasoro modes; string oscillator mode expansions [Zwiebach Chapter 9]

20080201: quantization of fields of spins 0,1,2 in LF gauge [Zwiebach Chapter 10]

20080206: first quantization of relativistic particle in LF gauge: Heisenberg vs. Schrodinger operators; Hamiltonian; matching up particle with field states; Poincare symmetry generators in LF gauge [Zwiebach Chapter 11]

20080208: first quantization of relativistic open string in LF gauge: Algebra of Virasoro symmetry generators; role of oscillators [Zwiebach Chapter 12]

20080213: quantum critical dimension and zero-point energy; constructing the open string quantum state space [Zwiebach Chapter 12]

20080215: Constructing the closed string quantum state space; Superstrings: worldsheet fermions, NS and R sectors, GSO projection [Zwiebach Chapter 13]

[reading week: no classes]

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Homework 1

Grade weighting

10%

Due date

Deadline: Wednesday 6th February 2008 before 2:15pm.

Lateness penalty: 3% per day up to a total of two weeks.

Drop-dead deadline: 2:15pm on Wednesday 20th February. Assignments handed in more than two weeks after the due date, without a relevant valid medical certificate or equivalent gold-standard excuse, will not be marked.

PROBLEMS


1. Zwiebach 3.9 and 3.10: gravitational field of point mass in one extra dimension [Relatively easy]
(3.9a) Find the gravitational potential of a point mass located at the origin in five noncompact dimensions.

(3.9b) Now put the fifth dimension on a circle of radius a and find the gravitational potential as an infinite series. (Hint: think method of images)

(3.9c) Show that, for distances much bigger than the compact dimension’s radius, r>>a, the four-dimensional form of the gravitational potential is recovered as an approximation.

(3.10a) Sum the series using the math identity in Zwiebach Q3.10 or your fave math reference.

(3.10b) Expand the analytic expression to find the leading correction at large radius to the four-dimensional answer. For what value of r/a is this correction a 1% effect?

(3.10c) Look in the opposite limit of small radius r<<a. What are the first two terms in the small-radius expansion of the five-dimensional potential? Is the leading term familiar?


2. Zwiebach 5.5: relativistic point particle in EM field [easy]
Synopsis: In proper time gauge, add the termpointparticleEMcoupling

to the geometric (kinetic) action for a free point particle,

pointparticle-kinetic

and derive (from first principles) the equation of motion following from the combined action. Prove that this equation reproduces the Lorentz force law in 3-vector form familiar from undergraduate physics.


3. Zwiebach 6.7: Open strings ending on Dp-branes of various dimensions [easy]

In a [flat] spacetime of dimension d+1, imagine a [lone] Dp-brane with p spatial worldvolume dimensions. Consider an open string ending on this Dp-brane. Let the p directions parallel to the Dp-brane worldvolume be labelled as the {x^i, i=1,…,p} and the orthogonal directions be {x^a, a=(p+1),…,d}.

(a) State the conditions satisfied by the curly-P_sigma. Treat separately the time {0}, {i}, and {a} components of curly-P_sigma.

(b) Prove that all boundary conditions (BCs) are satisfied for the case of the D0-brane (p=0).

(c) Prove that if the string ends on a D1-brane, the tangent to the string at the endpoint is orthogonal to the D1-brane, and the endpoint velocity is unconstrained.

(d) Prove that if the string ends on a Dp-brane with p>=2, either

(i) the string is orthogonal to the Dp-brane at the endpoint, and the endpoint velocity is unconstrained;

(ii) the string is not orthogonal to the Dp-brane at the endpoint, and the endpoint moves with the speed of light transversely to the string.


4. Zwiebach 7.6: Planar open string motion and cusp formation. [Harder]
Consider a relativistic open string in planar motion in the {x,y} plane. Let the string endpoints be attached to (x,y)=(0,0) and (x,y)=(a,0) where a>0. Use the general formalism from class for solving classical open string motion, with the vector function F(u) and the quasi-periodicity condition F(u+2sigma_1) = F(u) + (2a,0).

Use the solution ansatz from Zwiebach 7.5,

hw1-dFdu

and the fact that

a/sigma_1 = J_0(gamma),

where J_0 is the Bessel function of order zero and gamma may be assumed to satisfy

0 < gamma < pi/2.

Since J_0 is not a periodic function, the relationship between a, sigma_1 and gamma is unusual: open string motions corresponding to gamma and 2pi+gamma are not the same.

(a) Show that the instantaneous slope of the string is described by

hw1-Xprime1

where

hw1-beta

Show that at ct=sigma_1/2 the string is horizontal.

(b) Prove that the instantaneous (transverse) velocity of the string satisfies

hw1-1cdXdt

Note that at t=0 the string has zero velocity. Conclude that whenever gamma < pi/2 no point on the string ever reaches the speed of light. Moreover, show that for gamma =pi/2 the string midpoint sigma=sigma_1/2 acquires the speed of light when the string is horizontal.

(c) A tractable case is obtained for gamma=sqrt{2}(pi/2). Show that at ct=sigma_1/4 one point on the string reaches the speed of light. Examine the string at the slightly later time ct=sigma_1/3, show that there are two points that have the speed of light, and find the corresponding values of sigma. Analyze X-prime (partial_sigma X) as a function of sigma to show that the string has a cusp at each of these points. A cusp on a string is a point where the two outgoing string segments form zero angle. Equivalently, at a cusp the oriented tangent to the string reverses direction.

(d) Use your favourite mathematical software package to generate the picture of the string considered in (c) at various times (use numerical integration!). Assume that a=1 and verify that sigma_1 ~ 10.155. Show the string for ct=0, sigma_1/4 and sigma_1/3.


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Lecture 23 Jan

These are my lecture notes for 23 Jan.

The related chapter Z-bach, Ch.7, is a discussion of worldsheet coordinate parametrization for the relativistic string. In particular, the worldsheet spatial coordinate sigma is chosen according to two criteria:

  1. that sigma be perpendicular to the worldsheet time coordinate tau, and
  2. that the energy density of the string dE/d(sigma) be constant in this parametrization.

PS: Here is an older set of notes on the Noether and Goldstone Theorems (from my graduate Quantum Field Theory course of a few years ago). These notes contain a pretty clear discussion of Noether’s Theorem and also Goldstone’s Theorem, in the context of relativistic field theories. YMMV, but I hope you find these notes helpful. :-)

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Lecture 18 Jan

Lecture Notes

Synopsis

Today we talked about the equations of motion and boundary conditions for a classical relativistic string, in an arbitrary worldsheet coordinate system.

We found that the only two boundary conditions for open strings physically consistent with the classical equations of motion are

  1. Dirichlet (can be imposed on any or all spatial coordinates), where open string endpoints are stuck to particular constant values, OR
  2. Free Endpoint, where open strings leak no momentum off their ends.

We then noted that static gauge, a partial fixing of worldsheet coordinate invariance, is physically simple to understand because it aligns target space time with worldsheet time.

We next introduced the notion of the s parametrization, in which the worldsheet spatial coordinate is chosen such that ds=|dX|
where X are the spatial guys. In this particular choice, we found that the Nambu-Goto action simplified a great deal, to the point where it looked a lot like a string generalization of the familiar geometric action for the point-particle. In this s parametrization and in static gauge, we found out two physically interesting facts: the open string endpoints move perpendicular to the string and at the speed of light.

String Theory Strikes Back 

Please also read an excellent article by Prof. Michael Dine of UCSC in this month’s edition of Physics Today magazine [local PDF file]. In it, Dine explains brilliantly why string theory is very relevant at the dawn of the LHC era, and he also brilliantly debunks critics of the field (like popular-book criticism emanating from the general direction of Lee Smolin of the Perimeter Institute and some blogs…). N.B: this is a must-read article for anyone interested in the relevance of string theory to physics.

P.S.: Regarding Gary’s question:

Note: Gary’s in-class observation was right – it looks like choosing Dirichlet BCs tells us that our wee D-brane can’t move. But don’t let that fool us – if we wanted to kick our D-brane a little to see how it’d react, we’d obviously need to have a mechanism of kicking the D-brane! In other words, just like if we wanted to make a point particle move (say, under an electric field), then physically we’d need the kick of energy-momentum to come from somewhere… and so adding that into the story results in (inevitably!) extra term(s) in the effective action for the whole system. The action for the whole system would then include the D-brane of interest plus whatever we’re kicking it it with. This would be just like adding the electromagnetic coupling to the geometric action for the free particle so we can study interactions of particles with EM fields.

The Nambu-Goto action we’ve used for calculation so far is for free strings living in flat spacetime. We can and will handle more complex cases later on. Worldsheet reparametrization invariance (conformal symmetry) is the fundamental quantum symmetry principle; the equations of motion are consistency conditions. If there is more than just a free string living in flat spacetime in the picture, then more terms will naturally be there in the low-energy effective action. Quantum consistency is what dictates the low-energy effective action for strings, D-branes and stuff they couple to, not inspired guessing.

Once we’ve developed [light-cone] quantization technology, we’ll see very clearly that D-branes most definitely can move; they gravitate and do other stuff besides. The deep quantum consistency of string theory is what tells us how to write down the correct equations for D-branes (in motion or whatever) and their interactions with open and closed strings.

Homework thought exercise from a student question:

Can an open string have Free-Endpoint boundary conditions on one end and Dirichlet on the other? Is there anything inconsistent about that?

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How to Contact your Prof.

If you ever forget my email address or phone number, just jump on the web (as you presumably are now) and point your web browser to

This is my “business card” site, which lists my contact data for students (and colleagues) first.

PS: ap.io stands for Amanda Peet Input/Output :-)

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