For Winters!

Winter is here and so the holidays and breaks. Here, I include few papers that might be interested to you to read in this winter break. In no specific order. Theme- Random Matrices and JT gravity.

Some bonus recommendations ;)

  • Newly appeared paper by Ed Witten on Quantum field theory in curved spacetime (https://arxiv.org/abs/2112.11614). There are also lectured by him on the same on Youtube.
  • Anna Karenina by Leo Tolstoy.

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A time with Einstein

I simulated Albert Einstein with GPT-3. The best that I could. Here is the conversation we had. I have edited some stuff, I did not include anything, but all quite was fun.


Me: What is spacetime?
Einstein: Space-time is the four-dimensional fabric of the universe. It is made up of three spatial dimensions and one temporal dimension.

Me: Why do you think spacetime is important?
Einstein: I think spacetime is important because it allows us to explain the large scale structure of the universe.

Me: What is the general theory of relativity?
Einstein: Theory of general relativity is a geometric theory of gravitation that explains the force of gravity as due to curvature in spacetime.

Me: Could you think of a larger dimensional spacetime?
Einstein: It is hard to imagine a spacetime with more than four dimensions.

Me: What do you think of Poincare invariance?
Einstein: Poincare invariance is a symmetry of the laws of physics.

Me: Do you think our universe is symmetrical?
Einstein: I think that the universe is approximately symmetric, but I do not believe it is exactly symmetric.

Me: What is your view on quantum theory?
Einstein: I do not like quantum theory. I think that it is fundamentally incomplete, and I have a variety of objections to the standard interpretation of wavefunctions.

Me: Ok, why it is incomplete?
Einstein: I think that quantum theory is fundamentally incomplete because it does not include a dynamical spacetime.

Me: What do you mean by dynamical spacetime?
Einstein: A dynamical spacetime is a spacetime that evolves in time.

Me: So, you wrote a paper EPR. Was it because you think quantum mechanics is incomplete?
Einstein: Yes, I, Podolsky, and Rosen wrote a paper EPR because we wanted to point out that quantum mechanics was incomplete and need modifications.

Me: Did you read the Bell's paper comment on your paper?
Einstein: I did.

Me: Why you were searching for unified theories?
Einstein: I was trying to find a unified theory because I thought that the fundamental laws of physics were not fully understood.

Me: What do you think of the 2+0 gravity and Kaluza-Klein model?
Einstein: I think both are interesting and do not describe the real world.

Me: What do you think of free will?
Einstein: I do not believe in free will.

Me: What do you think of string theory?
(There was not any reply here)

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What's Happening

Here are a few hot topics in high-energy physics. Not in any order. Moreover, of course, they are biased from my eye-view of hep-th.


  1. Random Matrices
  2. Black Holes, Entropy of BHs and Entanglement
  3. D-Instantons
  4. Anti-de Sitter and Causality
  5. JT Gravity
  6. Conformal Field Theories Applications
  7. Strings/BHs Correspondence

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Complex Analysis: Analytic Functions, Cauchy-Reimann

Some basics of complex analysis. We will follow L. Ahlfors's Complex Analysis book. An analytic function is a complex-valued function with derivatives everywhere where function $f(x)$ is defined with an appropriate power series. Holomorphic functions are the same, with a different meaning. For an analytic function $f(z) = u+iv$, we write


$\frac{\partial f}{\partial x} = \frac{\partial u}{\partial x}+i\frac{\partial v}{\partial x}$

with the limit

$f^{\prime}(z)=\lim _{k \rightarrow 0} \frac{f(z+i k)-f(z)}{i k}=-i \frac{\partial f}{\partial y}=-i \frac{\partial u}{\partial y}+\frac{\partial v}{\partial y}$

from which we can extract

$\frac{\partial u}{\partial x}=\frac{\partial v}{\partial y}, \quad \frac{\partial u}{\partial y}=-\frac{\partial v}{\partial x}$.

These differential equations have a name; Cauchy-Reimann differential equations. (They have well-meaning in complex analysis, greatly in Reimann spheres, from my readings.) If one compute $|f(z)
|^2$, which is a Jacobian of $u$ with respect to $x$ and $v$ respect to $y$, one can extract from the Jacobian that $\Delta u$ and $\Delta v$ are harmonic functions as

$\Delta u=\frac{\partial^{2} u}{\partial x^{2}}+\frac{\partial^{2} u}{\partial y^{2}}=0$
$\Delta v=\frac{\partial^{2} v}{\partial x^{2}}+\frac{\partial^{2} v}{\partial y^{2}}=0$

and $u$ and $v$ satisfy the Cauchy-Reimann differential condition. $v$ is said to be a harmonic conjugate of $u$, $u$ is a harmonic conjugate of $-v$.

If $u(x, y)$ and $v(x, y)$ have continuous first-order partial derivatives which satisfy the Cauchy-Riemann differential equations, then $f(z)=u(z)+i v(z)$ is analytic with continuous derivative $f^{\prime}(z)$, and conversely.



Edit: If one wants to go at an advanced level (which sure one needs in theoretical computations), try Stephen Fisher's Complex Variables, as suggested by one friend.

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Renormalization Without the Infinities

It is a common misconception that renormalization is needed only when infinities are coming up. But R. Shankar beautifully tackles this in his textbook on Quantum Field Theory and Condensed Matter in chapter 11th. 


The central idea of renormalization is to do the computation by integrating out unnecessary mathematics, so we get good physics out of it. But a lot of good renormalization problems do not have anything to do with infinties. I will reproduce here one such example from the same book. Let us take a system $(a,b,c, \cdots,n; x,y)$, where $a,b,c,\cdots,n$ are parameters and $x,y$ are two variables. Calculating a partition function of such a system is easy. But what if we want to compute the partition function ignoring variable $y$. Such thing is achieved by writing a modified system $(a',b',c',\cdots,n')$

$Z(a',b',\cdots,n') = \int dx \left[  \int dy e^{-a(x^2+y^2)}e^{-b(x+4)^4} \right]$

$Z(a',b',\cdots,n') = \int dx e^{-S(a',b',c',\cdots,n')}$

where $S'$ is the action of the modified system. So

$e^{-S(a',b',c',\cdots,n');x} = \int dy e^{-a(x^2+y^2)}e^{-b(x+4)^4} \equiv \int dye^{-S(a,b,\cdot,n;x,y)}$ 

here we have created an effective action $S'$ of an effective theory. We did not eliminate $y$ by setting it zero, but we created an integral where we integrated out $y$ but got the same answer as the original theory. The second integral with integrated of exponential with Boltzman weight have interactions parts involving $x,y$. In the last we have modified the system in such a way that we do not need to figure out the coupling of $x$ and $y$, but we have set the fate of $x$ to itself.

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Gaussian Matrix (Random)

We will take a $4 \times 4$ random unitary matrix of Gaussian nature (Hermitian ensemble) -  generated from Mathematica.


with $det =$.

 Eigenvalues of the given matrix are computed below.


One may now do many things with this matrix, such as generating its Gaussian distribution. 

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Misconception between Bosonic String and Susperstring in RNS Formalism

There are many common misconceptions (or carelessness) that amateur string readers have. One of those is that bosonic string theory on worldsheet is for bosons, and superstring theory on superspace is for fermions (well, only fermions). This is technically wrong. Superstring theory has both bosonic sector (with Neveu-Schwarz - NS- boundary condition) and fermionic sector (with Ramond boundary condition). However, the NS bosonic sector (which uses the same $X^\mu$ worldsheet of the free bosonic theory of D=26) of Superstring is different from the bosonic theory in D=26. One of the things that differentiate the two is the presence of an extra oscillator in the former.  NS bosonic sector does not have the critical dimension $26$ but $10$.

In superstring theory, we add an extra wave-function $\psi^\mu$ which is related to $X^\mu$ by world-sheet supersymmetry (space-time SUSY is used in GS formalism). The fermionic sector (of course of Superstring) is also ghosts-free at $D=10$. And the Virasoro algebra of the free bosonic theory is replaced by the Super-Virasoro algebra.

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Random Matrices

I have been lately studying the random matrices and their application that widely defaults for the JT gravity. Though, random matrices need to be started with Wigner's idea of the random matrix in nuclear theory. Right now, random matrix theory can be considered an important subject, at least from my learning view. In the following (short), I present my rough ideas of random matrix theory, extracted from here.


Random matrix theory (RMT) is a classic example of statistical group theory in general physics. The most recent development for RMT is the equivalence of JT gravity with RMT, see here. From the correspondence of AdS/CFT, one learns that a bulk theory with gravity lives on the boundary of a quantum system. However, the equivalence of JT gravity is not given to a boundary theory (or a bulk theory). In fact, RMT shares the correspondence with JT gravity; hence JT gravity is dual to random matrix integral of Hamiltonian $ H $, where $ H $ is a random matrix.

(RMT is mainly concerned about groups' statistics, at least for us, whose applications are wide in physics, as indicated.)

Consider a matrix $ \sf M $, from linear algebra we know that $ \sf M$ holds eigenvalues $ {\sf {m}}_{ij} $ (for $ 2 \times 2 $ matrix). Suppose the elements of matrix $ \sf M $ are random variables, to which we say to obey some specific outlined properties. In that case, the study of those ($\mathsf{m}_{ij} $) eigenvalues are called the "random matrix theory'' problem. Now one can ask what the practical application of RMT is. Actually, there are many practical applications. Consider the well-studied example of the nucleus using these random matrices, which Wigner (and Dyson) developed. And the recent example of the success of RMT is JT gravity. I suggest the reader to read the most interesting book on this subject by  Madan Lal Mehta.


From a mathematical perspective, random matrices serve great as well. However, it tends that it is currently revolutionizing the physics. Nuclear physics had first exploitation of random matrices. And now, it is used as a tool in black hole information problems, JT gravity (see the Saad, Shenker, Stanford), and other statistics problems (include the pedastriation and all that researches).  The deformations of these matrices were done by Witten, and he also did the volume problems for the subject. 

Radom matrices can be classified into classes. See sec. 4 in this and Witten's paper on JT gravity. For a full study, consider the Mehta's book.

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Few Updates

Let us catch with some updates. 

  • Susskind has a good paper on de-Sitter space here. He has been pretty active in de-Sitter lately. One should first start with his and colleagues' paper on the causal patch and then follow up on his recent writings. (I recently saw a video of Susskind highly appraising Juan Maldacena here.)
  • I wrote a fine and short piece of introduction (and basically mixed up) article on field theory and beyond, which can be found here and here.
  • Subir Sachdev, TIFR, and IAS have organized a course on Quantum phases of matter. The lectures can be viewed at http://qpt.physics.harvard.edu/qpm/.
  • Breakthrough Prizes have been awarded https://breakthroughprize.org/News/65.
Ig Nobel Prizes are out, check it to chuckle a little.

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For Summer!

Here, I include some important papers (or books) which one (if not already) should read in this Summer. (Of course, I can miss many great which I have read or haven't).


  • Two-dimensional gravity and intersection theory on moduli space by Edward Witten - https://inspirehep.net/literature/307956. This work founds one of the pillar for later developments in JT gravity and Random Matrix theory.
  • Large N field theories, string theory and gravity by O. Aharony, S. S. Gubser, J. M. Maldacena, H. Ooguri, and Y. Oz - http://arxiv.org/abs/hep-th/9905111. One of the best introductions to AdS/CFT and Large N Correspondence (and Gauge-String duality).
  • S. Coleman, “Aspects of Symmetry: Selected Erice Lectures,” 1988.
  • J. H. Schwarz, “Introduction to superstring theory,” NATO Sci. Ser. C 566 (2001) 143–187, arXiv:hep-ex/0008017.
  • A. Eskin and M. Mirzakhani, “Counting closed geodesics in Moduli space,” arXiv e-prints (Nov., 2008) , arXiv:0811.2362 [math.DS]. - It is a highly important work among many by Mirzakhani.
  • P. H. Ginsparg, “APPLIED CONFORMAL FIELD THEORY,” in Les Houches Summer School in Theoretical Physics: Fields, Strings, Critical Phenomena. 9, 1988. arXiv:hep-th/9108028
  • M. B. Green, J. H. Schwarz, and E. Witten, SUPERSTRING THEORY. VOL. 1 and 2: INTRODUCTION. Cambridge Monographs on Mathematical Physics.
  • G. ’t Hooft, “Large N,” arXiv:hep-th/0204069. Large N is nowadays bread and butter, so you must buy it.
I must repeat that this list is arbitrary but sure are of great help to me.
Happy Reading! - Aayush

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KLT Relations

Kawai-Lewellen-Tye Relation, see here, is a perfect tool to make connections between amplitudes. The most general of them is the relation between a tree gravity amplitude (from Einstein-Hilbert action) and a gauge theory amplitude (from Yang-Mills). We can also relate the closed strings amplitude and open strings amplitude using KLT. (Many connections are there for closed strings algebra and open strings. From a conversation with Ed Witten; Ed - The simplest is that they can be computed in similar ways by integral representations that come from the open or closed string).


From the paper (recommended);


and same paper (sec II, a short review);


More papers on this subject; here, here, and here.

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Old Superstring Formalism

I wrote a very brief discussing note on superstring formalism that was developed in the early years. In the note, I discuss it with required algebra. However, an adopted model for superstrings is good than this one. You can read it from here:


Old Superstring Formalism - Pdf

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Non-criticality and Criticality

Though some papers promise to show the Lorentz invariance in non-critical string theory, I haven't found any strong evidence of it, yet. Except some papers claiming it to be consistent in some scenarios.  Evidently, the addition of longitudinal oscillators in lower dimensions is not harmful, however, we wait for a good scheme for non-critical string theory. (I also have no idea of eliminating anomalies and ghosts in superstring in non-critical dimensions.) We discuss the origin of $D=26$ (critical dimensions) in bosonic string theory.


Among some ways of proving the criticality, the most famous is by using $j_{\mu\nu}$ (Lorentz elements) - A method involving a very after-canonical quantization process of deriving critical dimensions can be found in Polchinski's volume. You can check if the action you have written for your strings (Polyakov action) is Poincare invariant. If they are Poincare invariant, then they are in critical dimensions. For bosonic string theory, it is $D=26$ and $D=10$ for superstring. One can find the critical dimensions for superstring by adding fermions using RNS. For M-theory, a close but not similar process can be carried out. If the theory is critical, then we should not fear the super-conformal ghosts that appear as central charges in algebras of string theory. In $D=26$, one can have the vacuum state as a tachyon, which is negative mass squared. In superstring theory, tachyons don't appear. Tachyons are unstable.

We can't talk much about non-critical theory, however, some models show good significance, for instance, $D \geq 4$, but too premature. Also, T-duality is only applicable for critical dimensions in super-string theory (I haven't encountered any support for non-critical dimensions for T-duality). Some good studies are holding for non-critical string theory with its application to AdS (not aware of recent development).


Edit: Paper by Polyakov also had a solution to the critical dimension from 1981 (the original subject of paper was on summation of random surfaces). And, there are also prospects of Liouville thoeries in non-critical dimensions.

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Unparticles and Unnuclear

In this short paper, I sum up the ideas of unparticle field theory (UFT). UFT is a scale-invariant theory. Georgi proposed it in 2007. Some slides (of earlier times) by him are available here on the subject. Despite being a wonderful field theory, it lacks experimental evidence. However, indirect shreds of evidence are possible through the following channels


.

There are more channels other than these. (For technicalities of these interactions, refer to papers.) UFT has a parameter  in the field equations. UFT is unlikely (for now) to be observed because it can be integral values, for instance, 1/2. How would the field theory look? 

In the case of  , UFT is just standard model field theory (these scalar theories are scale-invariant). For instance a UFT with the propagator 


 is phase-space (refer to any paper on UFT).  When , the propagator becomes


which is a familiar propagator in SM. There are many more interesting things about UFT that I cover in the paper with results. You should check first (if new to UFT) papers by Georgi, Tzu-Yiang Yuan, and Kingman Cheung. Georgi is also carrying interesting results in Schwinger's problems. 


Recently, a new term was dropped in this area by Hammer and Son. Unnuclear physics is a non-relativistic theory of unparticles. This EFT claims much more experiments than unparticle physics (which is a relativistic version). A recent talk by Dam Son emphasized the phenomenology of unnuclear physics, which is his next paper (to be released this month). A lot is going in this field. However, it is a newborn field, so a lot can't be said. 

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Vertex Operators and Conformal Mapping

We can use the Feynman diagrams to replicate the process of scattering with strings. For particle interactions, we can do Feynman diagrams (for , see this - just topologies). For strings, we can do the same; we call them "string diagrams." A closed string forming two closed strings is depicted by changing the point-particle by strings and word line by worldsheet.




The crossing line indicates (this one line is for collective dimensions. However, there should be definitive for each one) that there is not one for all Lorentz frame, unlike in point particle theory, but two. It can be interpreted that the point-particle Feynman diagram is just a limiting case of the string diagrams. Furthermore, one string diagram (with vertex function) can be deformed to a few particle Feynman diagrams. That is one of the reasons why there are not many string diagrams. Lorentz frames are also the reason for the absence of ultraviolet divergence because of independent defined Lorentz sites at interaction.

Similarly, one can do the one-loop of string diagrams as we do in point particle. But, the convenience and Lorentz issue demand something better. We do that by conformally mapping the string diagrams. In this case, we map it to a topological disk (genus-0)




Among the advantages of conformal mapping, one being that there would not be the h (associated with  ) integrals in the matrix calculations. But what about the conservation of quantum numbers after topological mapping? For that, we introduce vertex operators. In the conformal image, cross-markers indicate the strings (the top one shows the far past string, and the bottom two indicates the far future newly born closed strings). The marked area is for the vertex operator. We can introduce it with the symbol , where m is for an m-type particle. This operation is effortless in a 1+1  system, which indeed we are following. The  is the operator for local absorption and emission of string states. We can introduce another operator , which is for the re-parametrization of the mapping. While W operators account for Lorentz transformation, we must also take accounts of translation. That is how we reach a well-known translation operator


The final operator for emission and absorption becomes


We need to fix the residual gauge invariance for the special linear group (when calculating the M-point functions). Conformal mapping for open strings (in this case, it should be on the boundary of the disk) is done in similar ways, however, they are different.

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Veneziano Amplitude

In string theory, when we write the Feynman diagrams, we denote amplitude for open and closed string, as Veneziano and Virasoro-Shapiro amplitudes (a complex beta function) respectively (we will only discuss the former). Veneziano amplitude is an Euler beta function that obeys the crossing symmetry and looks*

where s and t are Mandelstem variables defined;
and $ \alpha(s) $ is Regge trajectory.

The amplitude is a result of the work on the duality between s and t channels. According to this duality, the sum of all the s channels and t channels should be equal. It was written for a model obeying the Regge trajectory which at the time was indicating not the string theory, but a QCD theory.  The Euler form of the amplitude can be written through expansions as**


because any beta function of the form
can be written as 

Note * has only one pole rather than two and ** is written in t poles. What we can do is writing ** in s poles, which then


And that is the duality. We can study various aspects of it by keeping t fixed or s fixed. This is done in the very first paper on this by Veneziano, here. Also, in integral representation, as like a beta function, this amplitude can be written as 
                  
                  
In large s and fixed t
                                               
it is valid for a complex large s plane unless one gets too close to the positive real line. This indicates that quantum corrections would be received by the imaginary part. In large s and fixed t, one can also write $A(s,t) \sim s^{\alpha(t)}$ (for linear Regge trajectory), and since in general Regge theory $A(s,t)\sim s^J$ where J is averaged (effective) angular momentum, we see  

$$\boxed{ J = \alpha(t)}$$


For a good understanding of this amplitude (or string theory), you can read Superstring Theory by Green, Schwarz, and Witten. Or Polchinksi's volumes.

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Half-Baked Problems with Quantum Mechanics

In quantum mechanics, there are many problems; the biggest of them (according to a group) is finding the first and initial state. We are talking about the initial state of the observable universe; it sounds cliche. But people believe that if we can find the initial state, we can determine the difference between the macroscopic and microscopic world. I have not any thoughts on that. However, as like many, my respect for quantum mechanics is just fundamental (and theoretical). When you do quantum mechanics, without any evidence of research, you will likely come to believe that 'what is true and what is wrong' is differently to be seen in the subject.


Just like the statistical mechanics, we have $\rho$ the density matrix in quantum mechanics. This looks like

which tells you the probability of each state into finding, the bracket notations used in this style is called projection operator. If you are a realist, you should not see this as a superposition, and in fact, it is not any superimposed thing. This $\rho$ being classical shouldn't be the problem. 


When we come to 'Copenhagen's Interpretation of quantum mechanics, which is heavily misguided in different ideologies, we can observe incompleteness and loss of determinism. The former and latter can be written to co-exist as 'no macroscopic evidence.' It is not entirely true. However, it is accepted that the interpretations can be completed by the completeness of matching the probabilistic theory to macroscopic lurches of evidence. Indeed, we would enjoy a version like this. Rather than this, the Copenhagen interpretation is widely celebrated as a successful interpretation.

_____________________


The reason these are half-baked problems that no one now cares about it. These problems are widely accepted as 'reality and fundamental.' Even when young people try to think about it, they fall into the prey of 'cancellation' and 'no go' which they say are occults of the subject. But, my stance is quantum mechanics is an achievement that we should sing from time to time.


Notes; A friend of mine shared with me an unlisted link of a talk by Weinberg at 'Standard Model at 50', in which he talks the same. And in fact, this post is inspired by his talk. 


https://www.youtube.com/watch?v=mBninatwq6k



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