@MarkMitchison I saw a question about operation on fermions. You left a comment but the user wasn't satisfied, and I can understand his objection. glance also tried, but again it's not exactly what the user asked. I thought on the issue and found it problematic. I looked in Ballentine's book, to which the user refers, and I was very displeased with the proof that I saw there. Maybe we can talk tomorrow. It's a strange situation and I don't exactly understand what's going.
@Sofia But let's assume that they don't like my answer. In my opinion what they are trying to do is a waste of time and I don't have much inclination to show them how to do it in detail.
@Sofia The best way to manipulate fermions in occupation number representation is taking the anti-commutation relations as a definition, and then writing the states as I did. Any other way is cumbersome and gives little insight.
@Sofia "Proving" the anti-commutation relations is an odd thing to want to do; they are part of the definition of the Fermi operators that makes them useful
I have been trying very hard to understand, I am reading Ballentine's book on this topic, but I need help:
I realized that I don't understand how many particle states work with the creation & annihilation operators $ C_a $ and $C_a^\dagger $ while trying to calculate $\{C_a,C_b^\dagger\}$.
I wi...
@MarkMitchison This. There's a reason they're called canonical - they are (more or less uniquely) defining the algebra of creation/annihilation operators.
@Sofia You are right that my comment does not at all answer the question as posed. Rather, I am trying to help the OP avoid wasting their time with a pointless exercise. This is speaking from fairly substantial experience with occupation-number representation ("seecond quantised") calculations with fermions.
The entire problem of that user is that Ballentine apparently didn't define the second-quantized notation properly, so there are factors of $-1$ floating around unaccounted for.
@ACuriousMind I forgot that the energy-momentum tensor isn't zero inside the torus :'(
It's a ghost torus!
@user1667423 (This is now correct.) If the spatial stresses in the torus can be neglected and the overall field is weak, then you can find gravitomagnetic equations.
@MarkMitchison let's talk tomorrow. The use has problem with an anti-commutator for which indeed, I don't see a correct proof. Maybe that anti-commutator rule is correct, but the user showed a problem and he doesn't want to let himself convinced in other ways, he wants to understand what's going with his particular problem. And in his place I would behave the same. So, let's talk tomorrow, can we? Now I go to sleep with no delay.
@Sofia As I said, I have no interest in this problem though. If the OP is not satisfied with the existing answers then I don't want to spend more time on it.
To better describe my question, do the following experiment:
Calculate x=12+26+67+71
Now you might have spent some time in getting the answer. You burnt sugar, you used up energy to get the solution. But due to the conservation of energy, energy doesn't vanish. Where did the energy you spen...
@0celo7 You can associate wavefunctional to states and pretend you're just doing QM for a long time. Also, all scattering amplitudes are just probabilities, after all.
For indications of a deep connection between the nature of quantum vs. classical probabilities with the (non-)commutativity of observables, see this answer
(Also, I think the SE is not the best thing to think of as the fundamental equation of QM. Heisenberg's equation of motion is so beautifully close to Hamilton's classical equation of motion that I find the Heisenberg picture much more natural to derive.)
@Danu Yeah, the rigorous procedure is geometric quantizatiion and highly tedious because it takes ages to get something that resembles a Hilbert space structure out of the phase space
@user1667423 Since the mass distribution is stationary, the quadrupole moment is independent of time. Therefore there are no gravitational waves. There should, however, be a frame dragging through the center, as you've drawn it.
user54412
You could imagine a bunch of point masses all rotating in the sense as you've drawn
user54412
Each one induces frame dragging as seen in the Kerr metric, and all the effects should add
user54412
2:31 AM
I suppose gravitomagnetism would give you the result more quantitatively, but honestly that's just a mess of equations, so I prefer to think about these things intuitively.
user54412
@ACuriousMind The philosopher in me is really disappointed, because a good philosophy community could have handled this just fine. The premise is logically flawed: If A is conserved, and we think A diminished, and we observe B increased, clearly B is A. I mean, that just doesn't make sense.
user54412
Fumbling something so simple is what gives philosophy such a bad rap
I mean the question "Is knowledge energy?" is not something I'd really want to see as a philosopher, either, but it is definitely more philosophy of knowledge than physics
user54412
2:41 AM
Random aside: The hardest thing about GR simulations is plotting the data that comes out of them. Seriously, it's almost like plotting packages were designed by people who don't transform their coordinates at the drop of a hat. And they always assume time is some global parameter that never mixes with space.
Indeed. Probably because time is energy and energy is knowledge
user54412
Actually, today I realized how awful my data dumps really will be. Everyone likes to plot black hole stuff in Boyer-Lindquist coordinates. But the right way to simulate black holes is with horizon-penetrating coordinates, which will have different surfaces of constant time from B-L.
user54412
So I have to dump a whole sequence of time-slices in code coordinates in order to construct a B-L time slice
In a picture or video of a numerical relativity simulation, such as a neutron star merger into a black hole, how do they set up their coordinate system? Lets take the point in a video corresponding to x=10km, y=20km, z=30km, t=1ms. Spacetime itself is distorted, in a very complex way, so how do y...
Can any body tell me the difference between nature letters and nature articles published by nature magazine. Are they both the same or different publication. If different where can i get nature letter archieve. This is a link to one nature letter article nature.com/nature/research/research_by_type.html
@Eka I am not entirely sure about Nature, but several Physics Journals also have a "Letter" issue, where only very short articles presenting an idea are published. So in Phys.Lett.X you will not find articles with 20+ pages, while Phys.Rev.B will also allow articles with 70 and more
@Neuneck Phys Lett and Phys Rev are different journals by different publishers (Elsevier, APS, respectively). Phys Rev has, as its most prestigious publication, Phys Rev Lett, which only allows for short publications, Letters. Note though that many of the others in the Phys Rev family have "Rapid Communications", whose length is also restricted.
From what I remember, Nature publishes both Letters and Articles and the former is one page shorter (I think the limits are 3 pages and 4 pages, respectively).
@MarkMitchison Mark, if you say that "Proving" the anti-commutation relations is an odd thing to want to do; they are part of the definition of the Fermi operators, then I'd like to learn a bit from your experience. I didn't have much to do with fermions and the anti-commutation relation, and I am quite worried with a strange thing that I saw there. Different proposals that I saw to overcome the problem, do not actually succeed to do so. So, if we can talk, I would be glad.
@alarge Dx major misconception on my part. That's what you get from always reading the arxiv version and picking quotes in the bibtex format from inspires.
At the time of writing, areas around the Northern Territory (TC Lam) and Queensland (TC Marcia) in Australia are in the path of severe cyclones (category 4 at the moment, with the Queensland one - TC Marcia predicted to reach category 5 - Category scales used for Australia and Fiji). These cyclo...
@Sofia If you construct a theory with Fermions and demand that the field and its conjugate momentum fulfill a commutation relation you will find that the spectrum is not bounded from below. This is also apparent in the Dirac equation, where people sometimes argue with a "Dirac Sea" in which all negative energy states are filled so that the Pauli exclusion principle bounds the spectrum.
@0celo7 This is the link. I am sorry it's only now that I saw your message.
@Neuneck I don't have enough experience with fermions. I have a problem with an anti-commutation relation which seems simply not true. I saw a proof which is taking people as fools and since the anti-commutation relation is one very often used, I would like indeed to clarify it as much as we can, and if we cannot I'll consider to apply to some specialist.
@Neuneck it's the $\{ C_a C_b^{\dagger}, C_b^{\dagger}C_a \} = \delta_{a,b}$. A frequently used relation.
@Neuneck if $a \ne b$ we should have $C_a C_b^{\dagger} = - C_b^{\dagger}C_a$. Well, it seems not true.
@Neuneck if you try to apply the operator $C_a C_b^{\dagger}$ to the state $|a>$, and if you try to apply $C_b^{\dagger}C_a$, you'll see that you don't get the same result just differing by a minus. What you get in the first case is a complication.
Yeah, just try to impose commutation relations and work out the commutator $\delta(x^0-y^0)[\Psi(x),\Psi^\dagger(y)]$. It will not be proportional to $\delta^3(\vec x - \vec y)$
In fact, you can do this 'in tandem' with the anti-commutator derivation
the derivations are identical until right at the end