@MarkMitchison well, that would depend on the initial rho, correct? Note, when I did these simulations, I had a wrong initial rho, but both times, it converged to 1/7...
@TanMath No, I am asking whether there is a term in the master equation describing population entering the system on a certain site. It is not to do with the initial state. If there is only loss and no gain, then the population on site 3 must vanish after long times. This is common sense, really, if you think about it for a bit.
@TanMath I have no idea, you need to check your code. If you have a sign wrong then you might be inadvertently pumping population into the system somewhere.
@MarkMitchison well, solving the lindblad equation is done by an external module.. I only have to put the hamiltonian, collapse operators, initial rho, and a list of times to evaluate rho(t) at...what part of that could go wrong?
could the hamiltonian being wrong affect the results? I am pretty sure the collapse operators are correct...
@TanMath That could go wrong in many, many places. Especially if you don't understand what the module is doing. But assuming the module is not faulty, the error is in your code. You need to carefully go through and debug.
@TanMath Generally one expects dissipative master equations in a complex system to have a unique steady state, independent of the initial state. In the presence of symmetries in the master equation, it is possible to have a degenerate manifold of steady states, so that the final state does depend on the initial state.
However, it is clear that no steady state of that master equation will feature non-zero population on sites which have a constant loss rate.
@bolbteppa I think the notion is not the same. The PDF you link leads to a non-central extension of the Lie algebra, while "my" twist is just real 2-cocycle - this classifies central extensions.
@MarkMitchison plus it was not explicitly stated that those two terms are in the system hamiltonain, in fact, the first equation defines the system hamiltonian so I wasn't sure...
@ACuriousMind I'm not sure but from browsing it looks like the discussion on that page up to the non-central extension is talking about the (un-complexified) lie algebra derived from the lie group, note the lie algebra from a unitary lie group is not unitary hence one needs to complexify, I think this is what he does when he says "In a similar fashion" and twists...
@ACuriousMind I think your book is taking the complexified Lie algebra coming from a Lie group and forming the twisted UEA of the complexified lie algebra, while my pdf is taking the (complexified? At least in section 2.7 it is complexified!) lie algebra of a Lie group and then twisting it by Gamma matrices?
@bolbteppa Yeah, the difference is what we are twisting by - my book twists by real numbers, yours by gamma matrices/some other algebra elements. The latter method is a more general notion of twists than the former.
Well Verizon's choice to eliminate 2-year agreements (which greatly subsidize the cost of new phones) likely isn't going to help Apple sales any (who's going to drop $600 for the phone when they can get cheaper ones that do the same thing?)
The Minkowski metric is the unique metric preserved by Lorentz transformations, and the Lorentz transformations follow essentially from the assumption of a maximal speed.
@0celo7 so the way Landau and Padmanabhan explain it is that you have, for a light ray, $c^2dt^2 = dx^2 + dy^2 + dz^2$ i.e. $ds^2 = c^2dt^2 - dx^2 - dy^2 - dz^2 = 0$, and then Padmanabhan actually beautifully proves that $ds^2 = ds'^2 \neq 0$ for the infinitesimal separation of two events in two frames by taking a Taylor expansion of one in the other, which establishes the importance of $ds^2 = g_{\mu \nu} dx^{\mu} dx^{\nu}$ in special relativity
There is a youtube video of this too I can find
From this you have Lorentz transformations as those transformations preserving $ds^2$, hyperbolic rotations...
I don't know anything other than this, if you have a nicer way to think about it
Note this idea comes immediately from the postulates of relativity and derives what a Lorentz transformation is
The computation and an amazing discussion is in the first (or at least the first 3) video of this course youtube.com/watch?v=EotEgl8MMaw based off his book and Landau
I had a look at Zee's example in the start of III.II, I think that example only shows the existence and invariance of the interval when $ds^2 = 0$, then in the next chapter he starts using it when it's not 0 as if it's invariant in those cases too...
@MarkMitchison Now, since the hamiltonian and dephasing rate are in cm^- natural units (I think), I need to convert the recombination and trapping rates to cm^-1 in natural units?
Okay cool, I need to think about how to explain what is iffy about what Zee does, but instantly I can see his example only holds for light rays, while the spacetime interval is defined to be invariant for any kinds of events
haha, so Zee's footnote warning is about just disregarding all logic when talking about the spacetime interval for light, and says you need Einstein's clock, but I think his example only holds for light between two spacetime events and only holds because he sneakily chose the same starting and ending point of space, while Landau/Padmanabhan's proof holds for all cases for all kinds of interactions
Section 2 of his CFT book (vol 2) but you should read section 1 as well, if his derivation in section 2 is a bit too tough then Padmanabhan's book and video does it out a lot better
@0celo7 Padmanabhan justifies the proportionality argument ($ds^2 = ads'^2$ in the equation between 2.4 and 2.5) by Taylor expanding $ds^2$ as a function of $ds'^2$, i.e. $ds^2(ds'^2) = b + ads'^2$ so that $b = 0$ because of them being equal for a light ray
@0celo7 One reason would be because equality of Taylor expansions does not mean equality of functions (There are functions with Taylor expansion 0 about a point which are non-zero, for example).
@0celo7 I'm not a smartass then, because I'm universally well-liked ;)
@0celo7 Definition of "I am universally well-liked": When you pick a random person that knows me, the odds that they will like me are far larger than that they will dislike me. As the number of persons that know me grows to infinity, the probability one of them dislikes me goes to zero.