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3:31 AM
i know we can taylor expand a function written in the form of $\langle x \vert a \rangle$, but is there a way to taylor expand a ket not projected into any basis? for instance to expand $\vert x' + dx' \rangle$
 
4:16 AM
I don't like advertising posts here, but I asked a question one week ago, and have yet to receive a satisfactory response. If anyone would mind taking a look, or at least upvoting the question so others can see it, that would be much appreciated.
2
Q: Interpolation of $H_{mix}$

DarkRunnerGiven two points $(P,T, H_{mix})$, how can I interpolate $H_{mix}$ between them? In other words, if I had two points $(H_1, P_1, T_1)$ and $(H_2, P_2, T_2)$, where $H_{mix}$ is the enthalpy of mixing, $P$ is the pressure and $T$ is the temperature, how would I interpolate between them? I started...

 
 
5 hours later…
9:08 AM
@Relativisticcucumber Well, you don't directly expand the ket but you can write $\lvert x+dx\rangle=e^{-\frac{i}{\hbar}\hat{p}dx}\lvert x\rangle$
Then expanding the exponential $\simeq\lvert x\rangle-\frac{i}{\hbar}dx\hat{p}\lvert x\rangle$
 
9:50 AM
In Coulomb scattering for when we are dealing with relativistic particles, the following equation was written: $\vec p^2=\beta^2 E^2$. It is said that $\beta$ is the velocity, but isn't beta= \frac v c$ and how do we come up with this eq: $\vec p^2=\beta^2 E^2$ ?
 
10:10 AM
@imbAF in natural units $c=1$ i.e. $\beta=v/c=v$
 
But how we reach the equalisation
 
What?
 
$\vec p^2=\beta^2 E^2$
 
Start from $E=\gamma mc^2$ and $\vec{p}=\gamma m\vec{v}$
Square the second one and divide side by side
 
I usually know
$E=mc^2$ and $E^2=m^2c^4+p^2c^2$
 
10:20 AM
You are missing a $\gamma$ factor in the first one, otherwise it's just the second equation for stationary objects
 
What? I don't understand that
 
That's the relativistic energy. The correct formula is $E=\gamma mc^2$
Which is equivalent to your second equation
The first one you wrote is the rest energy for a massive object $p=0$
 
10:37 AM
But gamma, is the 4 dimensional vector, with elements matrcies
right?
 
...no.
it's the Lorentz factor
 
No, the gamma matrices are a separate thing
Have you studied some relativity before delving into Dirac's equation? :P
 
Yes I ave
have
but that is the gamma, as the lorentz factor
 
It is
 
it is very rare to see $\gamma$ mean "the vector of $\gamma$-matrices"
$\gamma$ is the Lorentz factor, $\gamma^\mu$ are the matrices, there's usually no danger of confusion
in particular since most equations can only make sense with one of these meanings :P
 
10:51 AM
I am a bit confused
I know the following eq. about energy
$E=$\frac{p^2}{2m}$ classic expression
and $E=mc^2$ when the particle has no velocity and $E^2=m^2c^4 +p^2c^2$ which is the relativistic dispersion equation
I don't see at which point a gamma is involved here
 
@imbAF this is the same as $E=\gamma mc^2$
Just written in terms of different variables
 
which of the two
cuz there are two expressions and
 
$E^2=p^2c^2+m^2c^4$
 
$\beta=\frac{v}{c}$ and $\gamma=\frac{1}{\sqrt{1-\beta^2}}$
Ok
 
ACM won't like this sentence but it's the same expression written in terms of the lagrangian or the hamiltonian variables :P
 
10:57 AM
But I wasn't aware of this : $\vec{p}=\gamma m\vec{v}$
 
$L(x,v)=-mc^2/\gamma$ is a relativistic lagrangian for a free particle
$\partial_v L=p$
Doing the calculation you'll find that expression for the momentum
 
in here c=1 right?
 
If you will you can set it equal to one, nothing will change
$E(x,v)=v\partial_v L-L=\frac{mc^2}{\sqrt{1-\beta^2}}$ is the energy
And if you express it in terms of $p$ you will get the hamiltonian $H(p)=\sqrt{p^2c^2+m^2c^4}$
 
Ok I'll try to derive it with all these tips
@Mr.Feynman I did, thanks
One more thing, why do we consider rest mass once relativistic speed is relevant ?
Like $pc>>>mc^2$ so why even bother considering the rest mass energy, when for the classical case, where one can make the claim that the kinetic energy can be in the range of rest mass energy, here we do not consider it. It feels that we are doing the reverse
 
 
2 hours later…
1:25 PM
Oh wise souls of stack exchange what is he talking about in these pages?
 
2:16 PM
@Mr.Feynman ahhh yup this gives me what i was looking for. nifty - thanks !!
 
 
1 hour later…
3:27 PM
whats the point of the support rods in a telescope? if you had them removed you wouldn't get the diffraction spikes
 
 
3 hours later…
6:24 PM
The Markdown at the bottom of this meta answer doesn't work because it's wrapped in HTML; the desired rendering could be achieved by using HTML instead of Markdown (e.g. <a href=X></a> tags)
 
 
2 hours later…
8:51 PM
What motivates the position of the spinor indicies when we write a Dirac spinor as $$\begin{pmatrix}\psi_\alpha \\ \bar{\chi}^{\dot{\alpha}} \end{pmatrix}$$
i.e. why is one down and one up?
 
9:20 PM
I'm guessing, it might be related to covariant&contravariant spinors
Due to the fact that left and right Weyl spinors have different transformation laws
 
It's diffcult to tell what is a convention or not
In the Lagrangian, the other side could have the top one up and the bottom one down
 
Section 56 of L&L 3 discusses contravariant and covariant spinors if it helps
Though I'm not sure that is the problem
 
I think maybe it may be convention because dotted indices are contracted conventionally through $\psi^{\dot{\alpha}} \xi_{\dot{\alpha}}$ and undotted through $\psi_{{\alpha}} \xi^{{\alpha}}$
Or maybe the other way round
So it would make sense to have one up and one down
But it seems like it's impossible to deduce what is a convention or not
 
Thinking about the way Weyl spinors transform, either with a matrix or its complex conjugate, I'm getting convinced it's about covariant/contravariant
 
it's co-/contravariant relative to the fundamental rep of $\mathrm{SL}(2,\mathbb{C})$, cf. physics.stackexchange.com/a/743759/50583
 
9:32 PM
Here's one (after the fact) way to see it. First, take the convention that $\psi_a' = M_a \, ^b \psi_b$, so that $\psi'^a = (M^{-1})_b \, ^a \psi^b$, as the $(1/2,0)$ representation. Then $\psi_{\dot{a}} = (M^*)_{\dot{a}} \ ^{\dot{b}} \psi_{\dot{b}}$ and $\psi^{\dot{a}} = (M^{-1})^*_{\dot{b}} \, ^{\dot{a}} \psi^{\dot{a}}$.
From $P = p_{\mu} \sigma^{\mu}$, which is Hermitian, and $P' = M P M^{\dagger}$. We thus see $M \sigma^{\mu} M^{\dagger} = M \sigma^{\mu} (M^T)^*$ has matrix indices $M_a \, ^c \sigma^{\mu}_{c \dot{c}} M^*_b \, ^{\dot{c}}$, where you need to be careful writing $P M^{\dagger}$ in indices due to the transpose.
Thus one Weyl equation is $\psi^a i \sigma^{\mu}_{a \dot{a}} \partial_{\mu} \psi^{\dot{a}}$. To figure out the second one this way, you need to determine what $\overline{\sigma}^{\mu}$ is, the position of it's indices, and write the second Weyl equation, which I'll leave as a way to check all this
There are other arguments e.g. involving parity, and how spinors transform under $\mathrm{SO}(3)$, and I can probably think of something better with some effort
 
Oh, since $\Lambda_L=\exp(\frac{1}{2}\sigma\cdot(-i\theta-\eta))$ transforms left spinors and $\Lambda_R=\exp(\frac{1}{2}\sigma\cdot(-i\theta+\eta))$, we have that $\Lambda_R=(\Lambda_L^\ast)^{-1}$. It's that inverse that gives rise to the notation
 
Ah okay thanks
 
Mhh wait, something's off with my message
Yes, the complex conjugation is wrong
 
I am off by a literal factor of $1/2$ in deriving the general BRST generator $Q$ from something sensible...
 
 
1 hour later…
10:46 PM
How can I just define what $(\bar{\sigma}^m)^{\dot{\alpha}\alpha}$ is?
Can just define a random tensor to be anything e.g. $M_{\alpha \dot{\alpha}}=\begin{pmatrix} 4 & 5 \\31 &11 \end{pmatrix}_{\alpha \dot{\alpha}}$?
 
11:20 PM
Is
$$\psi^a i \sigma^{\mu}_{a \dot{a}} \partial_{\mu} \psi^{\dot{a}} = - \partial_{\mu} \psi^a i \sigma^{\mu}_{a \dot{a}} \psi^{\dot{a}} = \psi^{\dot{a}} i \sigma^{\mu}_{a \dot{a}} \partial_{\mu} \psi^a = \epsilon^{\dot{a} \dot{b}} \psi_{\dot{b}} i \sigma^{\mu}_{a \dot{a}} \epsilon^{ab} \partial_{\mu} \psi_b = \psi_{\dot{b}} i \epsilon^{ \dot{b} \dot{a}} \epsilon^{b a} \sigma^{\mu}_{a \dot{a}} \partial_{\mu} \psi_b = \psi_{\dot{b}} i \overline{\sigma}^{\mu,\dot{b} b} \partial_{\mu} \psi_b$$
(Ignoring a total derivative)
 
So you define $\bar{\sigma}^\mu = (\sigma^\mu)^T$?
where all indicies in the expression above are in the same place
@bolbteppa Why can't I just complex conjugate this. The indicies will just stay in the same place then
Something weird is going on
 
11:40 PM
No, I defined $\sigma^{\mu}$ in that equation
Using the convention that $\epsilon^{12} = \epsilon^{\dot{1} \dot{2}} = + 1$ we have $\epsilon = i \sigma^y$, which completely breaks our index convention, however using it we can write
$$\overline{\sigma}^{\mu,\dot{b} b} = \epsilon^{ \dot{b} \dot{a}} \epsilon^{b a} \sigma^{\mu}_{a \dot{a}} = \epsilon^{b a} \sigma^{\mu}_{a \dot{a}} \epsilon^{ \dot{b} \dot{a}} = i \sigma_y^{ba} \sigma_{a \dot{a}}^{\mu} i \sigma_y^{\dot{b} \dot{a}} = - i \sigma_y^{ba} \sigma_{a \dot{a}}^{\mu} i \sigma_y^{\dot{a} \dot{b}} = [(\sigma_y \sigma^{\mu} \sigma_y)^{b \dot{b}}]^T $$
i.e. $\overline{\sigma}^{\mu} = (\sigma_y \sigma^{\mu} \sigma_y)^T$
This qft stuff is all revised in supersymmetry so that's the place to go looking for a refresher
(So, in terms of explicit matrices, we have $\overline{\sigma}^{\mu} = (I,-\sigma^i)$ if $\sigma^{\mu} = (I,\sigma^i)$)
 

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