Let's say I am dealing with a factorized Hilbert space $\mathcal{H}_1 \otimes \mathcal{H}_2$. I want to generate the Lie group $SU(2) \otimes SU(2)$ consisting of all unitaries of the form $(U_1: \mathcal{H}_1 \rightarrow \mathcal{H}_1) \otimes (U_2: \mathcal{H}_2 \rightarrow \mathcal{H}_2)$. Can this be done by taking the direct product $\mathfrak{su}(2) \oplus \mathfrak{su}(2)$?
I feel I am not using standard notation... does $SU(2) \otimes SU(2)$ usually refer to local operators of the form $U_1 \otimes U_2$?
also I mean to continue...taking the direct product of the lie algebras and exponentiating elements in the resulting direct sum of lie algebras?
Other than using $\otimes$ instead of $\times$, I think I am using standard notation actually based on the wikipedia for direct product.
Look at this question: Does the universe have a center?. It is the original one. (original, unpopular)
Now, look at this one: Did the Big Bang happen at a point?. (duplicate, famous)
If you notice, the duplicate post has a comment by a moderator that redirects to the original post:
Now, the orig...
@Slereah What did you want to do, that you have to do this? You know that TikZ gives you freedom to use general vector coördinates, right, not just relative coördinates of objects?
question about dirac notation. if i want to write something like $ <A^\dagger v, B v> $ do i write $ <v \vert A^\dagger B \vert v> $ or$ <v \vert B A^\dagger\vert v> $
Why is that a problem? $\left<\phi|AB\psi\right>^*=\left<AB\psi|\phi\right>=\left<B\psi|A^\dagger|\phi\right>=\left<\psi|B^\dagger A^\dagger|\phi\right>$
my lecture is based on sakurai, my tutor refuses any kind of notation that is not 100% equal to what he has on his solutions paper. this is simply not using dirac notation with the three bars (as Sakurai uses it)
If you want the more complete version, A is an operator representable by a matrix, $\left|\phi\right>$ is a ket vector that is usually representable by a column vector, and the action of a matrix on a column vector is a column vector, and so $A\left|\phi\right>=\left|A\phi\right>$ always makes sense: matrix multiply vector equals vector.
Look, what you wrote as the usual mathematical proof, is not even correct. It should be
$\left<(AB)^\dagger\phi|\psi\right>=\left<\phi|AB|\psi\right>=\left<A^\dagger\phi|B|\psi\right>=\left<B^\dagger A^\dagger\phi|\psi\right>$ which then implies $(AB)^\dagger=B^\dagger A^\dagger$
If you want to go into greater detail, you can complex conjugate basically everything there, so then you can express them with the 2 bars.
But as you already wrote down in maths notation, this thing kinda requires the 1 bar version, not the 2 bar version.
@Slereah i have a follow up question to something you said a few days ago. so iirc, you said that $\sqrt{-g_{\mu \nu}\frac{dx^{\mu}}{d\lambda}\frac{dx^{\nu}}{d\lambda}}$ is a valid lagrangian when attempting to use lagrangian mech to get the geodesic equation. however, i see that the einstein-hilbert action is defined by $S_H = \int \sqrt{-g}Rd^nx$ so why, in the first case, do we not have to include $R$? [...]
[...] in that case i believe we are solving for geodesics of free, non-interacting particles, but this is still in a curved space-time, right?
im not really understanding. so R is the curvature essentially, right? so im trying to see why the first action doesnt have an R in it as the einstein-hilbert action does.
It is similar to how particles couple with the electromagnetic potential A, but the kinetic term of EM is the EM tensor
Or how classically the acceleration depends on the derivative of the potential, but the EoM is the Poisson equation, with the Laplacian of the potential
@Relativisticcucumber I think we first need be clearer that these are actions for two completely different physical systems
the "geodesic action" is an action $S_G[\gamma]$ on the space of paths $\gamma: I\to M$, the dynamical variable is the path of a particle, the metric is a fixed background here
the Einstein-Hilbert action $S_{EH}[g]$ is an action on the space of all metrics on a manifold, the dynamical variable is the metric itself, and there aren't any particles here
so the question "why does one of these include $R$ and the other doesn't?" is about the same as asking "why does the action for the trajectory of a particle in an electromagnetic field not involve the field strength tensor, while the action for electromagnetism with the EM field being the dynamical variable does?"
@Slereah I'm fairly sure there are several cults claiming we actually are pure energy; the GR sticks are probably part of the conspiracy to suppress the truth :P
@RyderRude Checkmate: I'm a Weinbergian and believe in the primacy of particles.
Neither QM nor QFT in their formalisms really come with an ontology attached, stop claiming they say such ill-defined things like "everything is a field"
the QFT formalism works regardless of what ontology, if any, you ascribe to an interacting state
"is" a proton three quarks? or "is" it a mass of sea quarks and gluons? or "is" it an "excitation in a quantum field"? You can argue that the answer to all of these questions is "Yes", but I find the last description the most unenlightening
is there any particle interpretation of the interaction region of scattering experiments?
@ACuriousMind the field ontology is unenlightening because it's more reductive, more fundamental. the particle description is best for the special cases
but when u r in the interaction region, there is no particle interpretation as even an option
yes, we can do physics without ever talking about an ontology. but if we r going to choose an ontology, the field ontology is the one that applies to all situations.
so i am just saying that it is superior to the particle ontology. im not saying that u r forced to think of an ontology
i can describe the interaction region's ontology using fields
while the particle ontology ceases to be an option
@ACuriousMind about your comments on my question (now deleted). I can choose any amount of time to move the blade through say a chunk of metal. There are lambda primes but they cancel on both sides. As for point 2. You need a finite force you have $1/ r \to \infty$ , the only chance you have is $ r \dot \to 0$
@MoreAnonymous my point was that the path of the knife can just be modeled as the trajectory of the knife point $t\mapsto (h(t),r(t))$. I do not understand what $\lambda(t)$ is supposed to represent
also you're right that you need $\dot{r}\to 0$ at $x=0$ for the forces to work (this is just the observation that the particle moving up the dome will reach the top with zero velocity), but what does this have to do with "infinite velocity"?
In astrophysics, spaghettification (sometimes referred to as the noodle effect) is the vertical stretching and horizontal compression of objects into long thin shapes (rather like spaghetti) in a very strong, non-homogeneous gravitational field. It is caused by extreme tidal forces. In the most extreme cases, near a black hole, the stretching and compression are so powerful that no object can resist it. Within a small region, the horizontal compression balances the vertical stretching so that a small object being spaghettified experiences no net change in volume.
Stephen Hawking described the flight...
In astrophysics and nuclear physics, nuclear pasta is a theoretical type of degenerate matter that is postulated to exist within the crusts of neutron stars. If it exists, nuclear pasta would be the strongest material in the universe. Between the surface of a neutron star and the quark–gluon plasma at the core, at matter densities of 1014 g/cm3, nuclear attraction and Coulomb repulsion forces are of comparable magnitude. The competition between the forces leads to the formation of a variety of complex structures assembled from neutrons and protons. Astrophysicists call these types of structures...
"We assume throughout that the matter composing the solar system can be idealized as a perfect fluid. For the purpose of most solar system experiments in the coming decades, this is an adequate assumption (see, however, section 9.2)"
Oh no
God there's a truckload of conditions for the classical limit