Why is there a k in Bondi k calculus?

  • Thread starter JUboy
  • Start date
  • Tags
    Calculus
k=const.}}\put(40.00,60.00){\vector(-1,1){0.12}}\put(40.00,60.00){\makebox(0,0)[cc]{}}\put(40.00,60.00){\makebox(0,0)[bc]{t' axis}}\put(30.00,40.00){\vector(1,1){0.12}}\put(30.00,40.00){\makebox(0,0)[cc]{}}\put(30.00,40.00){\makebox(0,0)[bc]{t axis}}\put(20.00
  • #1
JUboy
i have this question.we are being taught sr using bondi k calculus.it is said here that 2 observers A and B are moving with some relative velocity with respect to each other. observer A sends a signal at his time t and B receives it at B time t' .we say that t'=kt.my question is how do we know that such a linear relationship exists?is it an assumption or can it be justified on the basis of the postulates of SR?
 
Physics news on Phys.org
  • #2
JUboy said:
that t'=kt.my question is how do we know that such a linear relationship exists?is it an assumption or can it be justified on the basis of the postulates of SR?
The answer to first question is think "similar triangles"... a scaling argument.
The postulates of SR will suggest that t"=kt', reversing the roles of the emitter and the receiver. In this latter case, it's also "similar triangles [with a flip]".. but similarity in the Minkowski geometry sense: the "Minkowski-angle [rapidity] between a timelike ray and a lightlike ray is infinite".

Check out my posts in
https://www.physicsforums.com/showthread.php?t=113915

By the way, what text are you using?

(If you think about Lorentz Transformations from a matrix point of view, you'll find that its eigenvectors are the lightlike vectors and k and k-1 are eigenvalues.)
 
Last edited:
  • #3
can u elaborate on thesimilar triangles argument.
 
  • #4
JUboy said:
.it is said here that 2 observers A and B are moving with some relative velocity with respect to each other. observer A sends a signal at his time t and B receives it at B time t' .we say that t'=kt.my question is how do we know that such a linear relationship exists?
won't this linear relation hold if i use any other wave instead of light?
 
  • #5
In the first case:
draw a triangle with two future-pointing timelike-vectors from an event O, with a lightlike vector connecting the tips. Suppose that the elapsed time is t on source watch and the reception time is t' on the receiver's watch. Certainly, one can write: t'=kt, for that pair of t and t'. We want to show that we get the same k for any corresponding pair of T and T' on the respective watches.

Well... by drawing a magnified triangle from O with longer timelike legs, you can see that this triangle is similar to the original triangle. All corresponding [Minkowski-]angles are congruent. So, the legs are in proportion. That is, T=at and T'=at'... so, since t'=kt, we have (T'/a)=k(T/a)... or T'=kT... for any corresponding pair of T and T' on the respective watches.

In the second case, we are going to eventually exchange the role of source and observer. We can physically argue via SR that the same relation with the same k must occur. Geometrically [which is probably not done to introduce the idea... but to verify its consistency later], we first Minkowski-"rotate" ("boost") the original triangle so that the receiver is vertical [which changes no "Minkowski"-angles or -lengths]. Under a Minkowski-"rotation", events slide along Minkowski-"circles", which are hyperbolas on a spacetime diagram. If it's hard to visualize, play around with http://physics.syr.edu/courses/modules/LIGHTCONE/java/TwinParadox.html (select "equal intervals from O" and "Light Cone of Q").

Then reflect about the vertical axis... then scale upward so that the vertex off the vertical axis coincides with the vertex in the original triangle. This triangle is similar to the original triangle... so, t'' (on the original source-watch)=k t'(on the original receiver-watch).
[tex]
\]

\unitlength 1mm
\begin{picture}(55,90)(0,0)
\linethickness{0.3mm}
\put(20,10){\line(0,1){80}}
\linethickness{0.3mm}
\multiput(20,90)(0.12,-0.12){250}{\line(1,0){0.12}}
\linethickness{0.3mm}
\multiput(20,30)(0.12,0.12){250}{\line(1,0){0.12}}
\linethickness{0.3mm}
\multiput(20,10)(0.12,0.2){250}{\line(0,1){0.2}}
\put(15,30){\makebox(0,0)[cc]{t}}
\put(15,60){\makebox(0,0)[cc]{\gamma t}}
\put(15,90){\makebox(0,0)[cc]{t''=k(t')=k^2t}}

\put(55,60){\makebox(0,0)[cc]{t'=kt}}

\end{picture}
\[
[/tex]
 
Last edited by a moderator:
  • #6
JUboy said:
wont this linear relation hold if i use any other wave instead of light?

The linear relation should hold with any other wave.
However, I think you'll run into computational problems when you try to use the principle of relativity to get the important relation t''=k t', then try to relate k to the relative velocity. (Note that in the non-light case, the signal-speed of emission according to the emitter is different from the signal-speed of reception according to the receiver.)
 
Last edited:
  • #7
thanks robphy that was really helpful.
 
  • #8
JUboy said:
thanks robphy that was really helpful.

You're welcome.

But you never answered what text you are using...
 
  • #9
im not using any text we are being taught using the k calculus in college and we haven't been told to follow any particular book.
 
  • #10
A more detailed graphic and argument as to why k is constant. (If I ever get the latex to work :-( )Light travels in straight lines. So we can use geometry.

Trinagle (O,t,kt) and (O,2t, 2kt) are similar. Therefore we know that if light is emitted at the source at time t and arrives at the destination at time time kt, that light emitted at time 2t must arive at time 2kt - by geometry, and the fact that light travels in straight lines.

How do we know the triangles are similar? The included angle is obviously the same, and the two light rays (t,kt) and (2t,2kt) must be parallel. The light rays must be parallel because they must cover equal distances (x-coordinate distance) in equal times (t-coordinate times), meaning that their slope, dx/dt, must be the same.

The argument that light emitted from the destionationat time kt arrives back at the source at time k^2 t is based on the physical argument that the receiver and the transmitter can be interchanged, as there is no "absolute" motion, only relative motion.

We can use similar triangles again to show that

(O, kt, k^2t) and (O, 2kt, 2k^2t) are similar, completing the argument.

[tex]
\[

\unitlength 1mm
\begin{picture}(60.00,95.00)(0,0)

\linethickness{0.15mm}

\multiput(30.00,40.00)(0.12,0.24){83}{\line(0,1){0.24}}
\put(40.00,60.00){\vector(1,2){0.12}}

\linethickness{0.15mm}

\put(20.00,20.00){\line(0,1){20.00}}
\put(20.00,40.00){\line(0,1){20.00}}

\linethickness{0.15mm}

\multiput(20.00,20.00)(0.12,0.24){83}{\line(0,1){0.24}}
\put(30.00,40.00){\vector(1,2){0.12}}

\linethickness{0.15mm}

\multiput(20.00,50.00)(0.12,-0.12){83}{\line(1,0){0.12}}
\put(20.00,50.00){\vector(-1,1){0.12}}

\linethickness{0.15mm}

\multiput(20.00,40.00)(0.12,0.12){167}{\line(1,0){0.12}}\linethickness{0.15mm}

\multiput(20.00,40.00)(0.12,0.12){167}{\line(1,0){0.12}}
\put(40.00,60.00){\vector(1,1){0.12}}

\linethickness{0.15mm}

\multiput(20.00,80.00)(0.12,-0.12){167}{\line(1,0){0.12}}
\put(20.00,80.00){\vector(-1,1){0.12}}

\linethickness{0.15mm}

\put(20.00,40.00){\line(0,1){40.00}}
\put(20.00,80.00){\vector(0,1){0.12}}

\put(0.00,60.00){\makebox(0,0)[cc]{}}

\linethickness{0.15mm}

\multiput(20.00,30.00)(0.12,0.12){83}{\line(1,0){0.12}}
\put(30.00,40.00){\vector(1,1){0.12}}

\linethickness{0.15mm}

\put(10.00,30.00){\makebox(0,0)[cc]{}}

\put(18.00,30.00){\makebox(0,0)[cr]{T=t}}

\put(18.00,40.00){\makebox(0,0)[cr]{T=2t}}

\put(18.00,50.00){\makebox(0,0)[cr]{T=k^2 t}}

\put(32.00,40.00){\makebox(0,0)[cl]{T'=kt}}

\put(42.00,60.00){\makebox(0,0)[cl]{T'=2kt}}

\put(18.00,80.00){\makebox(0,0)[cr]{T=2k^2t}}

\put(60.00,60.00){\makebox(0,0)[cc]{}}

\put(30.00,40.00){\makebox(0,0)[cc]{}}

\linethickness{0.15mm}

\put(20.00,80.00){\line(0,1){10.00}}
\put(20.00,90.00){\vector(0,1){0.12}}

\put(20.00,92.00){\makebox(0,0)[bc]{T axis}}

\put(20.00,90.00){\makebox(0,0)[cc]{}}

\linethickness{0.15mm}

\multiput(40.00,60.00)(0.12,0.24){125}{\line(0,1){0.24}}
\put(55.00,90.00){\vector(1,2){0.12}}\put(55.00,92.00){\makebox(0,0)[bc]{T' axis}}

\put(55.00,70.00){\makebox(0,0)[cc]{}}

\put(60.00,60.00){\makebox(0,0)[cc]{}}

\put(85.00,75.00){\makebox(0,0)[cc]{}}

\put(80.00,85.00){\makebox(0,0)[cc]{}}

\put(18.00,20.00){\makebox(0,0)[cr]{O}}

\end{picture}

\]

[/tex]
 
Last edited:
  • #11
Here is a simpler diagram with the same argument as above. Thanks to robphy for helping me learn how to use the jpicedt tool and fix-up the latex so that it will display properly on the forum.

[tex]

\[

\unitlength 1mm
\begin{picture}(85.00,95.00)(0,0)

\linethickness{0.15mm}
\put(20.00,0.00){\line(0,1){90.00}}\linethickness{0.15mm}
\put(20.00,90.00){\line(0,1){0.12}}

\linethickness{0.15mm}
\put(20.00,90.12){\line(0,1){0.12}}
\put(20.00,90.24){\vector(0,1){0.12}}

\linethickness{0.15mm}
\multiput(65.12,90.24)(0.12,0.24){1}{\line(0,1){0.24}}
\put(65.24,90.48){\vector(1,2){0.12}}

\linethickness{0.15mm}
\multiput(40.12,40.12)(0.12,0.12){1}{\line(1,0){0.12}}
\put(40.24,40.24){\vector(1,1){0.12}}

\linethickness{0.15mm}
\multiput(60.12,80.12)(0.12,0.12){1}{\line(0,1){0.12}}
\put(60.24,80.24){\vector(1,1){0.12}}\linethickness{0.15mm}
\multiput(20.00,0.00)(0.12,0.24){375}{\line(0,1){0.24}}
\put(65.00,90.00){\vector(1,2){0.12}}\linethickness{0.15mm}
\multiput(20.00,20.00)(0.12,0.12){167}{\line(1,0){0.12}}
\put(40.00,40.00){\vector(1,1){0.12}}

\linethickness{0.15mm}
\multiput(20.00,40.00)(0.12,0.12){333}{\line(1,0){0.12}}
\put(60.00,80.00){\vector(1,1){0.12}}

\put(20.00,0.00){\makebox(0,0)[cr]{O\,}}

\put(20.00,20.00){\makebox(0,0)[cr]{A\,}}

\put(40.00,40.00){\makebox(0,0)[cl]{\,B}}

\put(20.00,40.00){\makebox(0,0)[cr]{C\,}}

\put(60.00,80.00){\makebox(0,0)[cl]{\,D}}

\put(20.00,92.00){\makebox(0,0)[bc]{T axis}}

\put(65.00,92.00){\makebox(0,0)[bc]{T' axis}}

\put(20.00,20.00){\makebox(0,0)[tl]{\beta}}

\put(20.00,40.00){\makebox(0,0)[tl]{\beta}}

\put(20.00,7.00){\makebox(0,0)[bl]{$\alpha$}}

\end{picture}

\]

[/tex]

In the above diagram, we have a stationary observer, represented by the T axis, who sends out light signals at events A and C.

We also have a moving observer, represented by the T' axis, who receives the emitted light signals at events B and D, respectively.

The time interval between events O and A according to the stationary observer is represented by [itex]\overline{OA}[/itex], similarly the time interval between events O and C is represented by [itex]\overline{OC}[/itex].

Similarly, the time interval between events O and B according to the moving obserer is represented by [itex]\overline{OB}[/itex], and the time interval between events O and D is represented by [itex]\overline{OD}[/itex].

We wish to prove that the ratio of the time intervals between received and transmitted events is a constant, i.e. we wish to show that

[tex]
\overline{OB}/\overline{OA} = \overline{OD}/\overline{OC} = k
[/tex]

where k is some constant. The fact that light travels in straight lines, and that the speed of light relative to the stationary observer is constant is sufficient to prove the above statement.

We do this by noting that the triangles AOB and COD are similar. We note that the angle marked [itex]\alpha[/itex] is common to both triangles. The two angles marked [itex]\beta[/itex] on the space-time diagram must be equal, as they are formed by the angle between a light beam and the T axis. Because the speed of light relative to the stationary observer on the T axis does not change with time, the slope of the light beam cannot change with time, hence the angle that a light beam forms with the T axis on the space-time diagram must not change with time.

Given that two angles of the triangles are equal, and that the sum of the angles of a triangle is 180 degrees, all three angles of the triangles must be equal, and the triangles must be similar.

Because the triangle are simlar, the ratios of the sides are constant. This proves the desired result that

[tex]
\overline{OB}/\overline{OA} = \overline{OD}/\overline{OC} = k
[/tex]
 
Last edited:
  • #12
i think that Bondi's k calculus has its origins in the radar detection and in the Doppler effect. its linearity consists in the fact that to one time in one reference frame corresponds a single time in another inertial frame
 
  • #13
bernhard.rothenstein said:
i think that Bondi's k calculus has its origins in the radar detection and in the Doppler effect. its linearity consists in the fact that to one time in one reference frame corresponds a single time in another inertial frame
Actually K-Calculus was the invention of E.A.Milne and found in his books "Relativity, Gravitation and World-Structure", 1935 (before the invention of radar), and its sequel "Kinematic Relativity", 1948, both Oxford at the Clarendon Press.

Milne's cosmology, kinematic relativity, was so-called because of its tight links to the kinematics of Einstein's Special Theory of Relativity.

Kinematics, in Einstein's Special Theory, is especially concerned with observers trying to make measurements of the behavior of objects moving in systems relative to themselves. According to Milne's understanding, these measurements could only be made by the observers signalling among themselves using light or other electromagnetic radiation, using clocks to time the signals.

Milne recognised that cosmology is only about observed photons that have arrived from the depths of space and asked of any cosmological concept, "How do we measure it?"

Given the hypothesis of the invariance of the speed of light Milne allowed equivalent observers only to send and receive light signals and measure time intervals using their own clocks. Distances were thus 'radar' distances, even before its invention.

As Bondi later remarked, “Milne's idea led straightaway to the radar speed gun!”

Garth
 
Last edited:
  • #14
k calculus

the diagram is presented by Asher Peres in Am.J.Phys.
 
  • #15
Yes - Milne uses a more primitive form of the diagram on page 48 of "Relativity, Gravitation and World-Structure", (1935).

Garth
 
  • #16
bernhard.rothenstein said:
the diagram is presented by Asher Peres in Am.J.Phys.
Are you referring to "Relativistic telemetry" by Asher Peres, Am. J. Phys. 55, 516 (1987) [keyword search for "telemetry" in http://scitation.aip.org/ajp/ ]? That paper doesn't show the full spacetime diagram [with the Minkowski-similar triangles with timelike legs] in my earlier post above... although it could be deduced from it.


Garth said:
Yes - Milne uses a more primitive form of the diagram on page 48 of "Relativity, Gravitation and World-Structure", (1935).

Garth

I only have the 1948 edition on my shelf. Thanks to your comment on Milne's work predating Bondi's, I've opened it up and looked at it in more detail. Indeed, the k-calculus calculations are there for special relativity [in the 1948 edition]... and Milne's approach can handle some additional cases.

However, in the 1948, "Fig 3 on p. 40" with "A's diagram and B's diagram" appears to be a pair of spatial diagrams, rather than spacetime diagrams. Is this true in the 1935 edition as well? If so, then Milne's diagram doesn't reveal the geometrical structure [i.e. the similarity of the triangles] in Minkowski spacetime... although it can be deduced from his algebraic equations.

(digression from this thread:
Milne is apparently interested in pursuing a modified theory of general relativity in which "galaxies constitute the natural frames of reference". Here are some webpages with some discussion:
http://world.std.com/~mmcirvin/milne.html
http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1996QJRAS..37..365W
http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1936ApJ...83...61R
http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1941Obs...64...11.
However, this digression is really off-topic.)
 
Last edited by a moderator:
  • #17
robphy said:
Are you referring to "Relativistic telemetry" by Asher Peres, Am. J. Phys. 55, 516 (1987) [keyword search for "telemetry" in http://scitation.aip.org/ajp/ ]? That paper doesn't show the full spacetime diagram [with the Minkowski-similar triangles with timelike legs] in my earlier post above... although it could be deduced from it.




I only have the 1948 edition on my shelf. Thanks to your comment on Milne's work predating Bondi's, I've opened it up and looked at it in more detail. Indeed, the k-calculus calculations are there for special relativity [in the 1948 edition]... and Milne's approach can handle some additional cases.

However, in the 1948, "Fig 3 on p. 40" with "A's diagram and B's diagram" appears to be a pair of spatial diagrams, rather than spacetime diagrams. Is this true in the 1935 edition as well? If so, then Milne's diagram doesn't reveal the geometrical structure [i.e. the similarity of the triangles] in Minkowski spacetime... although it can be deduced from his algebraic equations.

(digression from this thread:
Milne is apparently interested in pursuing a modified theory of general relativity in which "galaxies constitute the natural frames of reference". Here are some webpages with some discussion:
http://world.std.com/~mmcirvin/milne.html
http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1996QJRAS..37..365W
http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1936ApJ...83...61R
http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1941Obs...64...11.
However, this digression is really off-topic.)
You are correct, Milne's motivation was to reproduce the results of SR and generalise it to cosmology without conceeding space-time as a continuum. Therefore his diagrams only reflect 3D space with time as a parameter. In that sense his version of 'K-Calculus' is not geometric, only algebraic.

Garth
 
Last edited by a moderator:
  • #18
so would you say that k is constant because of homogenity of time?
 

FAQ: Why is there a k in Bondi k calculus?

Why is the letter "k" used in Bondi k calculus?

The letter "k" in Bondi k calculus stands for the wavenumber, which is a measure of the number of waves per unit distance. It is used to represent the frequency of a wave in the context of Bondi k calculus.

How is Bondi k calculus different from other forms of calculus?

Bondi k calculus is a specialized form of calculus that is used in the field of astrophysics to study the behavior of gravitational waves. It differs from traditional calculus in that it takes into account the curvature of space and time, which is a key component in understanding the behavior of gravitational waves.

What are the applications of Bondi k calculus?

Bondi k calculus is primarily used in the field of astrophysics to study the behavior of gravitational waves. It has been used to make predictions about the behavior of black holes, neutron stars, and other cosmic objects. It is also used in the development of new technologies for detecting gravitational waves.

Can Bondi k calculus be applied to other fields besides astrophysics?

While Bondi k calculus was originally developed for use in astrophysics, its principles and concepts can also be applied in other fields such as fluid mechanics, electromagnetism, and general relativity. However, its application in these fields may differ slightly from its use in astrophysics.

Is Bondi k calculus difficult to understand?

Like any other specialized form of calculus, Bondi k calculus may seem daunting at first. However, with a solid understanding of traditional calculus and a strong grasp of the principles of general relativity, it can be understood and applied effectively. It may require some time and effort to fully grasp, but it is a powerful tool in the study of gravitational waves in astrophysics.

Similar threads

Replies
7
Views
676
Replies
3
Views
1K
Replies
5
Views
1K
Replies
41
Views
3K
Replies
18
Views
2K
Replies
51
Views
3K
Back
Top