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8:00 AM
I have only seen a reference to Dirac's GR book once
It was in one of Those papers
On how to build wormholes FOR REAL
Because Dirac's book is one of the rare GR book to have the Bertotti-Robinson spacetime in it
which makes sense, I suppose
It's not a very relevant spacetime from a cosmological point of view, but it's a very physics spacetime to study
 
what's that spacetime like?
 
It's the spacetime generated by a homogeneous electric field
 
oh man
sounds kind of like Godel's onion
but worse
 
it's not a terribly complicated spacetime
but it's of limited interest
at least globally
 
okay I guess it would be like Godel's onion if it has a uniform E field and also was slowly spinning about an axis
anything with an infinite amount of energy is gonna be weird somehow
 
8:05 AM
Well, the FRW spacetime has infinite energy :p
and you're living in it
 
infinite action, not energy right?
or what, what's T in the FRW universe? it's not zero?
 
The stress-energy tensor is certainly not zero in the FLRW geometry.
There are energy density terms and pressure terms.
 
well. that is a lot of energy then
 
When you learn about the mathematics for physics, what are your strategies? How to attack them?
 
Step 1: Don't try to interpret every step of the workings with physical meaning e.g. $\langle \psi_a | \psi_b\rangle$ don't really have a physical meaning
Step 2: Think about how the equations are being simplified as you take account of physical constraints such as e.g. the size of the system, e.g. upper limit and lower limit of e.g. pressure etc.
 
8:16 AM
^what do you have against transition amplitudes
also ChoMedit that wasn't a very specific question
 
Doing global GR is the result of not growing out of said phase :p
 
lately I need to read about modular forms and it's very difficult to read the number theory literature, but this might not be what you're asking about
 
My question is for general areas of physics. I think there may be a consistent way to study the required mathematics.
 
I want to watch these videos on modular forms in string theory, skimming the first one he does things really nicely
 
@JohnRennie Well, Minkowski space is a FRW spacetime :p
 
8:19 AM
oh cool thanks
I've been watching Don Zagier's series
they're more mathematical, but he talks about some jones polynomial things
 
@bolbteppa Global GR is great
 
what do you mean by global GR
 
@Slereah also a Schwarzschild spacetime, a Kerr spacetime, etc, etc
 
@JohnRennie really most spacetimes have Minkowski space as a limit
Global GR is looking at the global properties of a spacetime
Rather than just the local properties encoded by the stress energy tensor
 
so you can look at topology, the conformal boundary, what else?
 
8:21 AM
first lecture he derives poisson summation and sets up a theta function and some more stuff, are those Zagier lectures insane
 
yeah he's nuts but he makes it work somehow
 
@RyanThorngren Causal structure, singularity analysis, Cauchy problem
 
only thing I don't like is he's very dismissive to his audience
 
Actually, what mathematical object is responsible for the topology of the spacetime in the context of GR?
 
that kind of stuff
@Secret The topology is
same as with every manifold
it's the atlas
Although if your spacetime is well behaved enough, this is equivalent to the Alexandrov topology
in which case you can say the metric is
 
8:23 AM
I'd ask what mathematical object encodes the causal structure!
 
@RyanThorngren also the metric!
There aren't that many mathematical objects in GR at its core
 
that's not what I mean
 
right, so for well behaved spacetimes, the stress energy tensor (which by Einstein Field Equations, is linked to the metric tensor) will have some control on the global topology of the spacetime?
 
of course the manifold with metric contains all the data
but if I ask you, "what's the causal structure of this spacetime?" how will you answer me?
 
There's a few equivalent statements for it
The most common one is that the causal structure is a partial order on the spacetime
$a \ll b$ if there's a future-directed timelike curve from $a$ to $b$
etc
 
8:26 AM
yeah that's good, though a very large piece of data
 
you can do it as the set of light cones for every points, too
or as the topology defined by causal diamonds
The causal structure has basically the property of being the same under conformal transformation
or should I say Weyl transformation
 
yeah
so there should be some conformal invariant way to specify it
 
you can even define spacetimes without manifolds or metrics
 
I heard of something like this for 2d spacetimes
 
simply from the causal structure
 
8:29 AM
where there are many simply-connected flat Lorentz surfaces
 
It's the approach used in causal sets for quantum gravity
 
Is there any considerable reason that why the temporal dimension is 1?
 
not unless you wear two watches
 
@ChoMedit well, observational evidence, for a start
Also matter isn't terribly stable with two time dimensions
 
That is very clear. By the way, I'm interested in your last sentence. Stability of the matter. What does it mean?
Or.. is there some reference for it?
 
8:32 AM
When you're working with multiple time dimensions, you have to solve differential equations with multiple times
Those are very badly behaved
Either there's no solutions, multiple solutions, or unstable solutions
2
 
determinism breaks down, if I recall?
 
that too
Also there's a lot of weird side effects
Like the photon isn't stable in 2 time dimensions
 
hey slereah take a look at this abstract tell me if it makes sense to you arxiv.org/abs/1601.06304 I thought it was an interesting take, but I wonder how a GR person would feel about it
 
@RyanThorngren Makes sense if he only considers conformal field theory, I suppose
if you want to know more about causal structures you can try this : arxiv.org/abs/gr-qc/0501069
a pretty good paper on the topic
 
cool thanks, I'll have a look
I think what he does is okay for effective field theory but you do need to understand the RG flow, which of course flows between CFTs
 
8:36 AM
The basic idea behind causal structures is that the set of causal structure is $$\text{Coset}(M) = \text{Lor}(M) / \text{Weyl}$$
With Lor the set of Lorentzian metrics
 
You can just define it as the equivalence relation of all weyl related metrics, although that's not the most satisfying definition
Also I think it doesn't work that well for spacetimes that are really badly behaved, IIRC?
Like I seem to recall that causal structures are only conformally related if you assume at least distinguishing spacetimes
 
hm I don't see what could go wrong
you mean in the sense of the partial ordering
?
 
I'm not quite sure what goes wrong, but the theorem proving that causal structures are identical for Weyl related spacetimes requires distinguishing spacetimes
i'm not aware of any counterexample for bad spacetimes, though
 
distinguishing seems like a reasonable assumption
otherwise you have points sitting on top of eachother or somethign
 
8:41 AM
I beware of "reasonableness" requirements :p
that's how you end up thinking all spacetimes are inextendible globally hyperbolic
 
haha well I think other spacetimes are above my pay grade, and are for the algebraic geometers or whoever to tangle with
basically I don't know how quantum mechanics can make sense without global hyperbolicity
 
it doesn't make a lot of sense :p
Usually it loses unitarity
Although then again
Even in globally hyperbolic spacetimes, it does
Ever tried to solve an electron orbitting a black hole?
 
using what, string theory? good luck :P
 
No, just QFT in curved spacetime
The Hamiltonian isn't hermitian :p
It corresponds to the electron getting lost in the black hole
 
yeah
that's not surprising
and probably not a good description of what actually happens
 
8:47 AM
true
Although when spacetime isn't globally hyperbolic, that's exactly what happens
You can just have particles popping out for no reasons
 
haha
that's why they created the naked singularity in half life
to see what would happen
and all the aliens came out
 
this is what happens
 
"The worry is illustrated in Fig. 3.1 where all sorts of nasty things - TV sets showing Nixon's "Checkers speech", green slime, Japanese horror movie monsters, etc. - emerge helter-skelter from the singularity."
 
lost sock, the ultimate embodiment of negative entropy
 
8:50 AM
hmm that's an interesting point, did anyone tried to calculate the entropy of a naked singularity?
 
what entropy
 
I don't know, does a naked (ring shaped) singularity has enough structure to talk about microstates of sorts?
 
I think the density matrix looks like $\sum_{anything and everything} |psi>_universe \otimes |anything and everything>$
so you're interested in log of the number of all things
which you should apply zeta fn renormalization and probably the answer is lost sock/2pi^2
 
I only know we can talk about something called soft modes on event horizon, but since naked singuarities lack event horizons, the information has to be encoded on it, I guess...?
 
I missed some bra's in there but hopefully you get the joke :P
 
8:54 AM
Also don't write raw text in tex :p
$|\text{Anything and everything}\rangle$
or $|\mathbf{Anything and everything} \rangle$
$|\mathfrak{Anything and everything} \rangle$
 
haha it doesn't compile for me anyway
 
what kind of tincan mathjax are you running
 
but if you really want to make a strong point nothing beats a paragraph of \mathbb
 
4
Q: Entropy of a naked singularity

resaypiAccording to the wikipedia article http://en.wikipedia.org/wiki/Naked_singularity: "Some research has suggested that if loop quantum gravity is correct, then naked singularities could exist in nature, implying that the cosmic censorship hypothesis does not hold. Numerical calculations and some ot...

Ok found something, so basically, since we cannot predict beforehand what is sprewed from the naked singularity, we have no way to count its microstates
 
honestly an empty tin of mathjax it seems
I've smoked all my mathjax
 
8:57 AM
Well there are some hints
A naked singularity may still have a mass
But of course nothing forbids that mass from running negative, if we're willing to have naked singularities, anything might go
 
can we make a naked singularity in AdS?
 
Well you can remove a point from AdS :p
But otherwise, it is geodesically complete
 
that's hardly an essential singularity
I mean in asymptotically AdS
 
Probably?
 
like you can make a black hole and look at the CFT dual state, which is mixed
 
8:59 AM
Although proving it sounds like a nightmare
 
there's some nice picture about the Ryu-Takayanagi screens not dipping into the event horizon
 
Like I suppose you could do the equivalent of the Kerr solution in AdS
and look at the extremal solutions
 
AdS is fucked up enough as it is, no need for singularities
it's already not globally hyperbolic
 
isn't it just a box
 
9:00 AM
Hell, in some definitions, AdS is nakedly singular
it's just that the naked singularity is the boundary at infinity
 
hm
well that's nice to imagine
 
But that's for the harshest definitions of naked singularities
 
turning the CFT cylinder into a twice punctured sphere
 
when a spacetime is nakedly singular if it's not globally hyperbolic
 
I have to decide what operators to put at the punctures
 
9:02 AM
Something probably random: Suppose we have a region of spacetime where random objects get sprewed out, I wonder if an observer can locally determine whether it is a region where determinism fails, or just one end of a CTC (thus what seemed to be a fountain of arbitrary objects is actually coming from another location in spacetime?)
Because if I recall correctly, both CTC and nondeterministic regions of spacetime violates unitarity, which caused me to wonder if there are ways to distinguish between them without the full information of the global structure of the spacetime
 
@RyanThorngren isn't a cylinder already a twice punctured sphere
 
just another way to look at things
 
I'm disturbed now you say ads is not globally hyperbolic because I've definitely heard people talking about cauchy slices for it
lol
I bet doing acid with NdGT would be great
 
AdS admits a foliation by spacelike hypersurfaces
But those are not Cauchy surfaces
You have timelike curves that go off to infinity at arbitrary $t$ and never go further
and vice versa, you have timelike curve coming from infinity that didn't exist before
 
9:12 AM
yeah that makes sense
but all the trajectories of massive particles stay bounded right
 
You can probably salvage it by requiring nothing to come from infinity I suppose
yeah massive particles are alright
 
I mean the theory is gapped from the perspective of the CFT
 
well, as long as you don't have any Rindler particles :p
 
okay you're right I'm talking about some specific theory there, type IIB string or something
I can see how it could go wrong otherwise
 
yeah fortunately AdS isn't that bad
I think it's fine if you just specify some boundary conditions at infinity
which is reasonable
 
9:15 AM
that's what I was trying to say with the punctures
but it wasn't very insightful
people like ads a lot where I hang around
 
you know me, I love spacetime
 
Except the Beem spacetime
 
and he investigates some of the most pathological of the spacetimes
 
and the Geroch spacetime
fuck those
 
9:17 AM
actually, thinking about another scenario:
 
$e^{i\pi} = -1$ test
fail
 
Giving a branching spacetime, then physics will become nondeterministic at the branching point, I think I need to figure how the causal structure there differs from a local event in a CTC
 
success!
how can spacetime branch
 
Non-Hausdorff manifolds
 
oh god why
haha
 
9:19 AM
It's a very mildly investigated theory
it's not pretty
cf here for instance
 
the aip link rotted
 
RIP
 
Error: The Requested Article is unavaiable
I think one question that might be potentially interesting for curation purpose (or whatever) is the classification of nonunitary spacetimes
 
what the hell is a non-unitary spacetime supposed to be
 
so far we have branching points, CTCs and naked singularities
(I am not sure if there is a formal term, its just something that pops up) Basically a region of spacetime where unitarity fails
 
9:23 AM
unitarity of what
 
so one cannot e.g. talk about the time evolution of a quantum field in such region?
Probability wise, it will not be conserved in such regions
That is, the probability of any physical process happening will fail to be conserved in such regions
such as near CTCs and naked singularities, particles will suddenly pop out or disappear to nowhere
(I really need to dig the correct terminology for what I have in mind of the intuitive notion of "a local region in the spacetime manifold where the observer is situated in" to express this properly)
 
"Let $(M,g)$ be a Malament-Hogarth spacetime containing a timelike half-curve $\gamma_1$ and another timelike curve $\gamma_2$ from point $q$ to point $p$ such that $\int_{\gamma_1} d\tau = \infty$, $\int_{\gamma_2} d\tau < \infty$ and $\gamma_1 \subset I^-(p)$. Suppose that the family of null geodesics from $\gamma_1$ to $\gamma_2$ forms a two-dimensional integral submanifold in which the order of emission from $\gamma_1$ matches the order of reception at $\gamma_2$.
If the photon frequency $\omega_1$ as measured by the sender $\gamma_1$ is constant, then the time-integrated photon frequen
Malament-Hogarth spacetimes are a meme!
 
9:38 AM
Gah, it is impossible to draw these spacetimes
This is a big incomprehensible mess
GR f*** up the notion of "distance between A and B" so much that I cannot triangulate where the concepts are located in a diagram
and that is why I found quantum mechanics slightly more intuitive, because I can at least draw a space of parameters to guide my calculations
> If the photon frequency ω1 as measured by the sender γ1 is constant, then the time-integrated photon frequency ∫p2ω2dτ as measured by the receiver γ2 diverges as p2 approaches p."
Ok then, so that means anyone who tried to read the solution of the halting problem will be fried by intense gamma rays instead
 
yes
"Suppose that $p \in M$ is a Malament-Hogarth point of the spacetime $(M, g)$ (that is, there is a future-directed timelike half-curve $\gamma_1 \subset M$ such that $\int_{\gamma_1} d\tau = \infty$ and $\gamma_1 \subset I^-(p)$). Choose any connected spacelike hypersurface $\Sigma \subset M$ such that $\gamma_1 \subset I^+(\Sigma)$. Then $p$ is on or beyond $H^+(\Sigma)$."
"There is nothing in the known laws of physics to prevent a false signal from emerging from the singularity and conveying the misinformation to $\gamma_2$"
 
Never seen $H$ before
 
Cauchy horizon
 
I see
I wonder if hypercomputation is doomed to fail for all spacetimes, as in whether there is a no-go theorem for hypercomputation...
 
it looks unlikely
 
10:03 AM
Guys how many divisions are there in a Kelvin Temperature scale?
 
It's a standard unit, so you just use the SI divisions
ie kilo, mega, giga, etc
 
I mean to get relation between Celsius and Fahrenheit scales, you do something like $\dfrac{T_{f}-32}{180}=\dfrac{T_{c}-0}{100}$
 
The division of Kelvins is the same as the celcius, only the origin point differs
 
I was wondering how to do this to get a relation between Kelvin and Celsius scales
 
So $T_k = T_c + 273.15$
 
10:08 AM
What's the lowest temp of Kelvin scale?
 
The lowest temperature is $0K$
 
273.15 right?
 
It is equivalent to $-273.15 ^\circ C$, yes
 
So 0 K is the origin for Kelvin scale?
 
Yes.
The division of kelvins is that there is $273.15$ kelvins between absolute zero and the triple point of water
 
10:12 AM
Okay so in the formula I wrote above, when I wrote 32 for the Fahrenheit scale, do I write it as the origin temperature of the scale?
 
I already gave you the formula above
 
@Slereah I know the formula! I was asking what's that 32 in the above formula I wrote, you see I'm trying to understand stuff
 
> On the Fahrenheit scale, the freezing point of water is 32 degrees Fahrenheit (°F) and the boiling point is 212 °F (at standard atmospheric pressure). This puts the boiling and freezing points of water exactly 180 degrees apart.[6] Therefore, a degree on the Fahrenheit scale is ​1⁄180 of the interval between the freezing point and the boiling point.
> According to a story in Germany, Fahrenheit actually chose the lowest air temperature measured in his hometown Danzig in winter 1708/09 as 0 °F, and only later had the need to be able to make this value reproducible using brine.[10] This is
> one explanation given why 0 °F is −17.78 °C, but the ammonium chloride cooling temperature actually is −3 °C, whereas that of NaCl is −21.1 °C; the other explanation is that he did not have a good enough brine solution to obtain the eutectic equilibrium exactly (i.e. he might have had a mixture of salts, or it had not fully dissolved). In any case, the definition of the Fahrenheit scale has changed since.
This is SO ARBITRARY for a 0 F definition
so, 180 is due to farenheit has 180 divisions and the freezing point of water is shifted up by 32
 
10:49 AM
"A modification of this example also serves to challenge the first dogma of observation. Create a past-truncated Minkowski spacetime by deleting all those spacetime points $r$ such that $t(r) \leq 2000 \text{B.C.}$"
What was so awful about that time that we have to delete it
"The past-truncated Minkowski model of Fig. 5.3 is, of course, very artificial (at least for those who do not subscribe to the creationist line of Protestant fundamentalism)."
 
11:12 AM
If $S = - m\int ds - e \int A_{\mu} dx^{\mu}$ is the action for a particle in an EM field, how does it change if you allow magnetic particles with charge, e.g. what happens to the Bianchi identity
 
Which Bianchi identity?
 
Yikes, you have to modify the EM field tensor apparently
A magnetic monopole is a hypothetical elementary particle in particle physics that is an isolated magnet with only one magnetic pole (a north pole without a south pole or vice versa). A magnetic monopole would have a net "magnetic charge". Classical theories of electromagnetism, represented by Maxwell's equations, disallow magnetic monopoles. Modern interest in the concept stems from particle theories, notably the grand unified and superstring theories, which predict their existence. Magnetism in bar magnets and electromagnets does not arise from magnetic monopoles, but from electric charges (i...
$dF = \frac{1}{3}(dF + dF + dF) = 0$
 
oh yeah
Basically the electric and magnetic fields become "symmetric" if you add a magnetic charge
 
'the Cabibbo–Ferrari relation'
'N. Cabibbo and E.Ferrari [2] have shown that if one introduce a second four-potential it is possible to eliminate the Dirac string.' I remember some waffle about Dirac strings
'The quantization of the theory remains a challenging open problem. The same can be said of its non-abelian extension'
 
11:28 AM
"In the philosophical jargon, we have a paradigm case of Hempelian deductive-nomological explanation"
the horror
 
what does that even mean?
 
Who knows
 
This is what I read: (incomprehensible) deductive (incomprehensible) explanation
 
11:45 AM
[continue on the british saying stuff]
29. Perfect with the following tone C#----F#, is the same as the british meaning
also 37 is really weird, how is that a punishment, you are wasting time on something that does not deserve a figurative "thank you" in any piece or form
because the truth is, the irresponsible won't even take note of that passive aggressive anyway
That's the problem of dealing with irresponsibles. Unlike trolls, you cannot make them regret their actions with the silence treatment
 
 
1 hour later…
12:55 PM
"Perhaps we have missed something. Suppose that Kurt tries over and over again to kill his grandfather. Of course, each time Kurt fails—sometimes because his desire to pull the trigger evaporates before the opportune moment, sometimes because although his murderous desire remains unabated his hand cramps before he can pull the trigger, sometimes because although he pulls the trigger the gun misfires, sometimes because although the gun fires the bullet is deflected, etc. "
Why does Gödel hate his grandfather so much
 
I'm confident that there are no magnetic monopoles. The electron has an electromagnetic field, not an electric field. IMHO it's missing the trick of electromagnetic unification to say it has electric charge and then say some other particle might have magnetic charge.
 
shoo shoo @JohnDuffield
 
I'm confident there are no wormholes either. IMHO if you've ever read David Finkelstein's 1958 paper you'll appreciate there are significant issues with it. And of course with the 1935 Einstein-Rosen paper.
 
Jesus that's a poorly OCR'd paper
 
I'm fond of quoting Einstein, but I don't quote from the Einstein-Rosen paper.
 
Could we make a magnetic monopole? Not in a fundamental particle sense.
 
Yes, there are objects similar to magnetic monopoles in condensed matter physics
They occur in superconductors, from what I can remember
 
You could make a very long solenoid.
One end of it is a magnetic monopole.
 
@JohnDuffield Could we call that magnetic monopole? It has its own pair even though it is very far away...
 
This paper doesn't really say anything new on wormholes, at least with modern eyes
 
1:18 PM
@ChoMedit : it isn't really a magnetic monopole.
@Slereah : when it comes to wormholes, I think this Einstein quote is worth noting: "it is easy to show that both light rays and material particles take an infinitely long time (measured in "coordinate time") in order to reach the point".
 
Well for the Einstein-Rosen bridge, obviously
Since they are joined at their event horizon
 
0
Q: Can this Q be reopened for answering?

StilezWhat could happen if we collide two subatomic particles with an energy of 39TeV? Or could we ever reach 40TeV? Closed as too broad, but - see comments - there is scope for a good answer. I'd have written more (times, energies), but comments aren't the right place for it.

 
If it takes an infinitely long time to reach the event horizon, it takes forever to cross the bridge, so you can never ever cross it. So it isn't a bridge.
 
Well yes
 
Besides Einstein and Rosen and Finkelstein were talking about particles, and particles aren't wormholes in any shape or form.
 
1:22 PM
Nobody is pretending that the Einstein-Rosen bridge is traversible.
I am aware.
You seem to be under the impression that those are mysterious issues that physicists aren't aware of
Those are all pretty well known facts of general relativity.
 
@Slereah : some people are suggesting that wormholes are traversable, when that goes against the grain of what Einstein said.
 
He seems to be back on word salads
Let's discreetely withdraw
 
I accidentally hit ENTER above. I've since corrected it.
 
Nobody is suggesting that the Einstein-Rosen solution is traversible.
and almost nobody is even suggesting that traversible wormholes are physical.
 
But some people are suggesting other wormholes are.
 
1:26 PM
Yes, which doesn't go against what Einstein said, as far as I'm aware.
His argument was fairly focused on the Schwarzschild metric
 
See what Kip Thorne advocates. He's one of the authors of MTW.
 
I'm well aware of Thorne's work, yes
 
IMHO the Schwarzschild metric is crucial. IMHO Oppenheimer and Snyder got it right with their 1939 paper on continued gravitational attraction. It ties in with what Einstein said. What Thorne says doesn't.
Gotta go. Sorry.
 
Same old Duffield
 
Instead of equations and derivations, names of authors and old essays are used to derive results :p
 
1:36 PM
Worst part being that these are fine little old papers
This isn't even a case of old papers being wrong
just unrelated to the matter
Not that I particularly believe wormholes are physical either, but whatever incoherent argument is trying to come through JD probably isn't the reason why
Nobody even really thought about traversable wormholes until the 70's or so, so it's pretty unlikely that papers from the 30's will say much on the issue
 
@bolbteppa lmao
I'm going to use and abuse that statement
 
Also really Oppenheimer-Snyder isn't a great paper to make a point about physically realistic models since it's not at all physically realistic :p
Dust collapse models are easy to deal with but they're not v. good
 
It probably is actually using the kind of thinking you'd use in math and physics, just in that fatally flawed 'argument from authority' language instead of the language of math
 
They tend to produce naked singularities
 
Poor guy, I tried to encourage him to study math once at least :(
 
1:44 PM
A bold attempt
 
Maybe Newton's Principia is wordy enough but with the jist of calculus and physics, a good start to ween off the quoting famous authors as a compromise :p
 
Newton's principia is really not a great place to learn math
It's from the era when using Euclid's geometry for almost everything was still the trend
It's not very readable by modern standards
 
Yeah it's terrible, but I remember buying the huge blue one before any other book thinking it was the davinci code of math and well...
 
This is the right place to learn calculus
 
1:46 PM
Isn't there some Marx calculus theorem haha
 
It's a nice book to have for historical reasons
but I wouldn't recommend calculus from Newton or algebra from Diophantes
 
I think he was part of the whole rigor/infinitesimal arguments before Weierstrass
 
Marx? Well, no, he wasn't aware of Weierstrass's work
But he got a good bit far himself
He was mostly learning mathematics in his last few years
 
I really don't know why the tumblr people are so in love with Marx, really
Since he was a white straight bourgeois man
You'd think he would be the worst thing
 
My sense is it's sycophants trying to say 'oh he did great things in THE calculus', but I have no idea tbh
The Mathematical manuscripts of Karl Marx consist mostly of Karl Marx's attempts to understand the foundations of infinitesimal calculus, from around 1873–1883. A Russian edition edited by Sofya Yanovskaya was eventually published in 1968, and an English translation was published in 1983 (Marx 1983). According to Hubert C. Kennedy, Marx "[...] seems to have been unaware of the advances being made by continental mathematicians in the foundations of differential calculus, including the work of Cauchy." In the same text, Kennedy says "While Marx's analysis of the derivative and differential had no...
 
1:49 PM
Ah Cauchy not Weierstrass my bad
He didn't do any breakthroughs
He was just attempting to understand calculus more rigorously
 
aren't we all
 
the differential was an elusive concept then
 
I wonder what was the big problem that made people realize that infinitesimals didn't work
 
You quickly run into trouble if you think about $dy/dx$ as a "fraction of infinitisimals"
I think $d^2y/dx^2$ doesn't play well at all with the chain rule
 
Hmm I know people say that stuff, but I think Euler's old calculus book was using differentials the way we do more or less, and DeMorgan and all these guys, and Leibniz was using them in some form, it seems like (comparatively) really complicated fourier series things or uniform convergence etc really kicked these guys into rigor, but I could be wrong
 
1:57 PM
$$\frac{d^2y}{dx^2} \neq \frac{d^2 y}{du^2} \left ( \frac{du}{dx} \right)^2$$
 
You have to add $(dy/du)(d^2u/dx^2)$ to the right
That's where the fraction thing starts to fall apart
 

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