hm, so if we include the identity with the pauli sigma matrices, it seems like we generate all 2x2 hermitian matrices. then if we exponentiate the identity with the sigma pauli matrices, do we still get SU(2)?
Oh my, I suddenly remembered something that puzzled me a year ago. In order for the coupled Maxwell action to be gauge-invariant, $\partial_\mu j^\mu=0$ has to be true off shell
@ACuriousMind this is what i had read in the "causal perturbation theory" approach. They were trying to sideline the path integral itself and just writing down the essential properties that they want from the path integral.
I was thinking more about the approach of actually properly defining the integral
Glimm and Jaffe wrote a book about how to do that in the 2d and some 3d cases but I'm not aware of anyone succeeding in extending this to 4d or even arbitrary dimensions
see this answer of mine for how the mathematically rigorous path integral actually works
@RyderRude so? That doesn't mean "take this vaguely defined continuum limit" defines a measure on the space of field configurations of the continuum theory in any mathematically rigorous sense
there's a lot of rigorous math involved in making sure discrete approximations and algorithms actually converge to the desired continuum limit
it's pretty easy to put some equation "on a lattice" and then write code that solves the discrete version on the lattice that just produces garbage instead of the actual solution for certain inputs
I once spent about a month writing Monte-Carlo code from scratch and my grand achievement was in the end that all the observables went to zero in the continuum limit
turns out there was a little bug in the description the course had us follow so while the algorithm looked okay, the way in which it scaled when you added points to the lattice just made stuff vanish on larger lattices
in another case I tried to reproduce results from some paper from the 70s and also just got mostly nothing, to this day I don't know if my implementation was buggy or the algorithm they described didn't actually work
(to be fair I didn't really care about that one after the course was over since there were plenty of newer results with other methods available in that area)
I think the lecturers didn't consider that "programming knowledge" as a prerequisite in most other physics courses meant something like being able to write a few lines of Python scripts
In QFT simulations, does the problm come from choice of the grid structure, or the numerical computation techniques? I expect it to be the latter
Or maybe both
I think there's not much choice in the grid structure tho, beyond the lattice size
Im just making sure that, conceptually, i can spend my life thinking of QFT as a theory on a rectangular grid.. even tho it doesnt work for practical computations
@ACuriousMind but this sentence of urs is making me think that there r bad choices of the grid structure
So i cannot think about it in terms of a rectangular grid, even conceptually
@RyderRude it's not about the grid structure, it's about how you discretize your equations to work on that grid
simple example: what do you do with a derivative? it needs to become a finite difference but there essentially are infinitely many of these finite differences that converge to the derivative in the continuum limit
but some of them may be good and others may be bad choices
e.g. you can discretize a unitary time evolution equation in a way that isn't unitary anymore for finite steps (this problem is classically solved by symplectic integrators).
While your discrete equation then still converges to the continuum equation in the limit, your solutions might "lose/gain energy" (or normalization or whatever) in each time step, so that they are pretty useless if you care at all about the original conserved quantity of your equation
this is all pretty generic numerics stuff and there's known rigorous solutions to most of these problems, but it shows that "just put it on a lattice and let a computer do the math" is still a far more involved and less straightforward procedure than non-computational physicists and their handwavy continuum limits tend to suggest
Do non-unitary and non-anti-unitary operators really have no place in quantum?
I am thinking okay so you want to use unitary (or anti-unitary) operators to essentially preserve probability. but surely there is some phenomena which includes changes in probability which can then be modeled by acting with a non-unitary operator?
for more context: i just started reading nielson and chuang's QI/QC book and they say that a quantum logic gate must be a unitary operator acting on your state, and i am trying to understand why it must be unitary
@SillyGoose but in the context of quantum information and quantum gates: A quantum gate just changes the state of a qubit to another state of a qubit. The total probability for the qubit to be in any state must remain 1
don't take this as some deep statement that there are never non-unitary operators in this context or whatever, they're just saying that what a quantum gate does is usefully modeled by unitary operators
@SillyGoose we usually do not change Hilbert spaces
the Hilbert space is supposed to be the space of all possible states of your system
if you can leave it you messed up the part about "all possible states" :P
heh but isn't it possible that your hilbert space changes over time. i guess depends how you define your system. since if you define your system as this cubic centimeter of space no matter what fills it at each time t, then your hilbert space will change with time in general? but maybe that is an unusual definition of a system
hm but if your system is so large like all space in europe and you would like to characterize such space, then it would help to take representative samples as representing your system
U wud b doing some very weird theory if the sample space changes with time. One example i can think of is a particle in an expanding box. But then, the correct way to think of it is to consider the entire real line as the unchanging hilbert space, and then modeling the expanding box using an infinite potential
@ACuriousMind Is it sufficient to just say that we need to make sure that whatever wavefunction represents the system we need to ensure that the system is sufficiently "large" so that it goes to zero at the boundaries of the system?
I have a P.hD entrance interview in 2 months. I have been specifically advised to study basics and focus on conceptual understanding. Also questions will be majorly asked from all areas of Physics. ( specially core subjects like QM, Electrodynamics, StatMech and also
Solid State physics, Nuclear ...
formally, when we want elements of the group SU(2) to act on vectors in a hilbert space, we still have to define a group action, right? it is just that matrix multiplication gives rise to a natural group action?
The above is the Källén–Lehmann spectral representation but without the fourier transform from $\mathbf{r}$ to $\mathbf{k}$ I think i.e. just with $t \rightarrow E$
Shows that rel QFT and non-rel QFT are essentially the same
what if we specialize to the hamiltonian? is there any way to distinguish it from other operators?
in particular, let's say we are given a hilbert space and a hamiltonian over the hilbert space. why should operators isospectral to the hamiltonian also be identified as being the hamiltonian?
i mean i guess from one perspective it is the same operator and all you are doing is changing basis by unitarily conjugating the hamiltonian.
again, position and momentum are isospectral, so $p^2$ (the free particle Hamiltonian) and $x^2$ are isospectral, too
but no one would claim that $p^2$ and $x^2$ should be "identified as being the Hamiltonian" of the free particle
but if you just look at this as the theory of abstract operators on a Hilbert space, then the Fourier transform provides an isomorphism between the $p^2$ Hamiltonian and the $x^2$ Hamiltonian, i.e. if you know how one of these systems behaves then you know how the other behaves
so the point about isospectrality is, I think, less that you should think of all systems with isospectral Hamiltonians as "the same" and more as "alike" in the sense that if you understand how to solve one of them then you know how to solve all of them