What does d represent in the context of \(\frac{dX}{dY}\) in Relativity?

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The discussion focuses on the meaning of "d" in the context of the derivative notation \(\frac{dX}{dY}\) within the framework of calculus and relativity. Participants clarify that "d" does not represent a separate quantity but is part of the derivative, which signifies the rate of change of one variable with respect to another. The term "infinitesimal" is highlighted as an appropriate descriptor for the small changes represented by "dX" and "dY." The conversation also touches on the linguistic challenges faced by non-native English speakers when discussing mathematical concepts.

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  • #31
Just want to add one thing.
I just realized that writing sin(x+h)-sin(x) = sin(h) is somewhat forgiveable.
But, writing cos(x+h)-cos(x) = cos(h) is really unforgiven. Should have remembered it "religiously" like the above post said.
 
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  • #32
Stephanus said:
Yes, sorry. Not d, but h.
##lim_{h \rightarrow 0} \frac{sin(x+h)-sin(x)}{(x+h)-(x)}##.
the (x+h)-(x). It is in the form of ##\frac{f(a)-f(b)}{a-b}##, right.
Should have change the letter d.

and this one is what I think that doesn't makes sense, see below.
##lim_{h \rightarrow 0} \frac{sin(h)}{h}##.
##lim_{h \rightarrow 0} \frac{sin(h)}{h} = 1##, a fact that is proven in most calculus textbooks. It's not immediatedly obvious, but you can check that it is reasonable by evaluating ##\frac{sin(h)} h## for smaller and smaller values of h (in radians).
Stephanus said:
[Add: could have written ##lim_{d \rightarrow 0} \frac{f(x+d)-f(x)}{d}##
But "d" here doesn't have any meaning right. It's just a variable.
But in this case, ##V^{\mu} = \frac{dx}{d\tau}##, now in this context, d has a meaning.
In your first example above, d does have a meaning -- as you say it's a variable.
In your second example, d by itself has no meaning, but ##\frac{dx}{d\tau}## means the derivative of x with respect to ##\tau##. By definition ##\frac{dx}{d\tau} = \lim_{h \to 0}\frac{x(\tau + h) - x(\tau)}{h}##

Stephanus said:
Just want to add one thing.
I just realized that writing sin(x+h)-sin(x) = sin(h) is somewhat forgiveable.
Why? This is not true.
Stephanus said:
But, writing cos(x+h)-cos(x) = cos(h) is really unforgiven. Should have remembered it "religiously" like the above post said.
I don't see the difference here. Neither one is true.
 
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  • #33
Mark44 said:
##lim_{h \rightarrow 0} \frac{sin(h)}{h} = 1##, a fact that is proven in most calculus textbooks[..]
Yes, this is a FACT!. I don't argue about it either.
Mark44 said:
Stephanus said:
I just realized that writing sin(x+h)-sin(x) = sin(h) is somewhat forgiveable.
Why? This is not true.
Stephanus said:
But, writing cos(x+h)-cos(x) = cos(h) is really unforgiven. Should have remembered it "religiously" like the above post said.
I don't see the difference here. Neither one is true.
Come on Mark114, give me some slack :smile:
##lim_{h \rightarrow 0} sin(h)## is almost zero, too. But of course ##lim_{h \rightarrow 0} sin(h) ≠ (sin(x+h)-sin(x))##
And of course ##cos(h)## is a light year away from ##cos(x+h)-cos(x)##
While ##sin(h)## is, I could say, in the neighborhood of ##sin(x+h)-sin(x)##, that's why I made a mistake with the statement above. sin(dx) while what I meant is d sin(x)
 
  • #34
Mark44 said:
In your second example, d by itself has no meaning, but ##\frac{dx}{d\tau}## means the derivative of x with respect to ##\tau##. By definition ##\frac{dx}{d\tau} = \lim_{h \to 0}\frac{x(\tau + h) - x(\tau)}{h}##
Oh.
Thanks, that helps me much in understanding SR.

Btw, about this ##\frac{dx}{d\tau}##. As you know in SR (Special Relativity) they often use X/T as their function not T/X (or Y/X) as in real 'math'.
That's why I made an error by saying gradient is X/Y, while what I meant is Y/X.
Of course in 'math', the gradient for vertical length is undefined, but in SR a vertical line as you know, is a rest frame.
While in SR, the horizontal line is undefined, velocity is instant, but in 'math' a horizontal line is Y = n, the gradient is zero.
 
  • #35
Stephanus said:
Yes, this is a FACT!. I don't argue about it either.
Come on Mark114, give me some slack :smile:
##lim_{h \rightarrow 0} sin(h)## is almost zero, too.
No, not almost zero. ##\lim_{h \to 0} \sin(h)## IS zero.
Stephanus said:
But of course ##lim_{h \rightarrow 0} sin(h) ≠ (sin(x+h)-sin(x))##
And of course ##cos(h)## is a light year away from ##cos(x+h)-cos(x)##
While ##sin(h)## is, I could say, in the neighborhood of ##sin(x+h)-sin(x)##, that's why I made a mistake with the statement above. sin(dx) while what I meant is d sin(x)
 
  • #36
Mark44 said:
No, not almost zero. ##\lim_{h \to 0} \sin(h)## IS zero.
I'm sorry Mark44.
if ##lim_{h \to 0} \sin(h)## is zero, how can
Mark44 said:
##lim_{h \rightarrow 0} \frac{sin(h)}{h} = 1##
I think ##lim_{h \to 0} \sin(h) = h##. and also tan(h) = h :smile:
 
  • #37
Stephanus said:
I'm sorry Mark44.
if ##lim_{h \to 0} \sin(h)## is zero, how can
Mark44 said:
##lim_{h \rightarrow 0} \frac{sin(h)}{h} = 1##
As I said in a previous post, this limit is proved in many calculus textbooks.
Stephanus said:
I think ##lim_{h \to 0} \sin(h) = h##. and also tan(h) = h :smile:
No, both of these are wrong. After you take a limit involving h, h will not appear in the result.
What is true is that for small h, ##\sin(h) \approx h## and ##\tan(h) \approx h##, but both limits you showed above are zero.
##lim_{h \to 0} \sin(h) = 0##
and ##lim_{h \to 0} \tan(h) = 0## as well.

Before attempting to study advanced physics topics, you should get a calculus textbook and study it, or study it in an online course..
 
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  • #38
Stephanus said:
I think ##lim_{h \to 0} \sin(h) = h##. and also tan(h) = h :smile:

This makes no sense since on the left side, ##h## is a dummy variable, while on the right it appears to be a real number.
 
  • #39
Stephanus said:
Of course in 'math', the gradient for vertical length is undefined, but in SR a vertical line as you know, is a rest frame.
While in SR, the horizontal line is undefined, velocity is instant, but in 'math' a horizontal line is Y = n, the gradient is zero.

You probably don't want to use the word gradient here...
 
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  • #40
micromass said:
You probably don't want to use the word gradient here...

To be more explicit:

In English-language math terminology, "gradient" is a concept from multivariable (vector) calculus, usually in three dimensions.

When we refer to the inclination of a line on a two-dimensional graph, e.g. a spacetime diagram for x and t in SR, we use the word "slope."
 
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  • #41
jtbell said:
To be more explicit:

In English-language math terminology, "gradient" is a concept from multivariable (vector) calculus, usually in three dimensions.

When we refer to the inclination of a line on a two-dimensional graph, e.g. a spacetime diagram for x and t in SR, we use the word "slope."
Yeah, I"m an Indonesian and in high school time, we used the word "gradien", no "t" there :smile:
But that was 30 years ago. I don't know what the word now.
And in space time diagram for an accelerated world line, this "slope" is the velocity at that particular time?
Can I ask here.
In ##Y = 4X + n##, the "slope" is "4"? Please confirm, so I can understand the explanations in SR Forum.
Thanks.
 
  • #42
Stephanus said:
And in space time diagram for an accelerated world line, this "slope" is the velocity at that particular time?

This is sneaky... :-p

In classical (non-relativistic) physics we always draw these diagrams with t on the horizontal axis and x on the vertical axis. The slope is dx/dt which is indeed the velocity, v.

However, in relativistic physics, we customarily draw spacetime diagrams the other way around: x on the horizontal axis and t on the vertical axis. The slope is dt/dx which is the reciprocal of the velocity, 1/v. I don't remember why people started doing it this way. Someone in the relativity forum probably knows.
 
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