A scientist’s transmitter emits a wavelength

In summary: However if the observer is accelerating away it could possibly outrun the absorbtion of the photon, but it would need......a very fast detector, or a very short time interval between emission and absorption. ...a very fast detector, or a very short time interval between emission and absorption.
  • #1
ramcg1
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A scientist’s transmitter emits a wavelength of very long wave electromagnetic radiation. We call him One and he watches his wave move through the universe at c.

Another scientist, call him Two, approaches One at very nearly c.
Two moves directly at One’s wave and nearly dies of fright when he sees a very high energy gamma ray approaching. Fearing possible cell damage and malignant cancer he turns on his magnetic deflector.

Just before the gamma ray reaches the magnetic deflector it spontaneously disintegrates into an electron / positron pair. The design of the magnetic deflector is such that the electron and positron are separated in the vacuum of pace and now moving in a plane perpendicular to the direction back to One.

One is scratching his head trying to work out how his very long wave turned into an electron / positron pair.

Later the electron and positron collide and the resultant gamma ray returns towards a dismayed One.

Where did the extra energy come from?
 
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  • #2
ramcg1 said:
Two moves directly at One’s wave and nearly dies of fright when he sees a very high energy gamma ray approaching. Fearing possible cell damage and malignant cancer he turns on his magnetic deflector.
That is impossible.
The space-time interval between an approaching photon and an observer is always zero.
 
  • #3
ramcg1 said:
A scientist’s transmitter emits a wavelength of very long wave electromagnetic radiation. We call him One and he watches his wave move through the universe at c.

Another scientist, call him Two, approaches One at very nearly c.
Two moves directly at One’s wave and nearly dies of fright when he sees a very high energy gamma ray approaching. Fearing possible cell damage and malignant cancer he turns on his magnetic deflector.

Just before the gamma ray reaches the magnetic deflector it spontaneously disintegrates into an electron / positron pair. The design of the magnetic deflector is such that the electron and positron are separated in the vacuum of pace and now moving in a plane perpendicular to the direction back to One.

One is scratching his head trying to work out how his very long wave turned into an electron / positron pair.

Later the electron and positron collide and the resultant gamma ray returns towards a dismayed One.

Where did the extra energy come from?

Hint: Model the process as a collision (see nits). What happens to Two's velocity after the collision with the gamma ray?

Various nits: Two wouldn't see the gamma ray coming, magnetic fields don't deflect gamma rays (they would deflect electrons or positrons), single photons in free space can't decay into an electron/positron pair unless they collide with something (energy and momentum must be conserved, which is not possible unless there is something else for the photon to interact with).
 
  • #4
ramcg1 said:
Two moves directly at One’s wave and nearly dies of fright when he sees a very high energy gamma ray approaching.

How does Two "see" the gamma ray approaching, before it meets him?
 
  • #5
MeJennifer said:
ramcg1 said:
Two moves directly at One’s wave and nearly dies of fright when he sees a very high energy gamma ray approaching. Fearing possible cell damage and malignant cancer he turns on his magnetic deflector.

That is impossible.
The space-time interval between an approaching photon and an observer is always zero.

I think you mean to say that the interval between the emission event and reception event of the photon by the observer is zero. Intervals are between events, not (say) worldlines.

Of course, this is a technical way to say that there is no way to "react" to an approaching gamma ray since nothing [in particular, information about the emission event] outruns light.
 
  • #6
robphy said:
I think you mean to say that the interval between the emission event and reception event of the photon by the observer is zero. Intervals are between events, not (say) worldlines.
Right.

But note that as soon as a photon was emitted in the direction of the observer then in the observer's frame of reference, using Einstein synchronized clocks, it has already been absorbed. :smile:
 
  • #7
MeJennifer said:
Right.

But note that as soon as a photon was emitted in the direction of the observer then in the observer's frame of reference, using Einstein synchronized clocks, it has already been absorbed. :smile:

Are you saying that the target observer determines the emission event to be simultaneous [i.e. assigns the same time coordinate t (in accordance with his wristwatch)] with the absorption event?
 
  • #8
robphy said:
Are you saying that the target observer determines the emission event to be simultaneous [i.e. assigns the same time coordinate t (in accordance with his wristwatch)] with the absorption event?
If we assume the observer uses Einstein clock synchronization then the answer is yes. Both the emission and the absorption of the photon are on the observer's plane of simultaneity.

However if the observer is accelerating away it could possibly outrun the absorbtion of the photon, but it would need to accelerate forever.
 
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  • #9
MeJennifer said:
If we assume the observer uses Einstein clock synchronization then the answer is yes. Both the emission and the absorption of the photon are on the observer's plane of simultaneity.

Hopefully, you realize that, in a nice spacetime like Minkowski spacetime, two distinct events that are simultaneous according to some observer are spacelike-related, whereas two distinct events on a photon's worldline are lightlike-related.

What is true is that both the emission and absorption events are on the past light cone of the absorption event [where the photon meets the observer].
 
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  • #10
robphy said:
Hopefully, you realize that, in a nice spacetime like Minkowski spacetime, two distinct events that are simultaneous according to some observer are spacelike-related, whereas two distinct events on a photon's worldline are lightlike-related.
Yes I realize that.
Is there anything I wrote that might contadict that? :confused:

robphy said:
What is true is that both the emission and absorption events are on the past light cone of the the absorption event [where the photon meets the observer].
Some would possibly say that issue seems to be a bit beyond the scope of run of the mill relativity.
But I would love to see, in a new topic, some proof of that assertion. :smile:
 
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  • #11
MeJennifer said:
Yes I realize that.
Is there anything I wrote that might contadict that? :confused:

Yes.
Distinct emission and absorption events of a photon can't both be spacelike related [if they are simultaneous for some observer] and lightlike related [if they are events of a photon].
 
  • #12
robphy said:
Yes.
The emission and absorption events can't both be spacelike related [if they are simultaneous for some observer] and lightlike related [if they are events of a photon].
The sub-lightspeed particle that emits the photon is indeed spacelike related to the observer, however that is not the case for the emitted photon. On the plane of simultaneity you will notice that both the temporal distance and spatial distance between the emitted photon and the observer is zero.
 
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  • #13
MeJennifer said:
robphy said:
What is true is that both the emission and absorption events are on the past light cone of the the absorption event [where the photon meets the observer].

Some would possibly say that issue seems to be a bit beyond the scope of run of the mill relativity.
But I would love to see, in a new topic, some proof of that assertion. :smile:

Take a look at Ellis and Williams "Flat and Curved Spacetimes" p. 48
to see the discussion of the past light cone vs the spacelike plane of simultaneity ("world map")... in ordinary Minkowski spacetime.

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  • #14
MeJennifer said:
That is impossible.
The space-time interval between an approaching photon and an observer is always zero.
Why is that?

Pete
 
  • #15
pmb_phy said:
Why is that?

Pete
Because, conform the Minkowski metric, the length of the photon's wordline is always zero, so then it follows that the distance between each point on this line and the space-time event that constitutes the absorbtion must be zero as well. :smile:
 
  • #16
MeJennifer said:
Because, conform the Minkowski metric, the length of the photon's wordline is always zero, so then it follows that the distance between each point on this line and the space-time event that constitutes the absorbtion must be zero as well. :smile:
What do you mean by "conform the Minkowski metric"??

What you said whas this
The space-time interval between an approaching photon and an observer is always zero.
A photon lies on a null geodesic and the spacetime interval between all photons on the same null geodesic is zero. So what you're saying is that the photon is on the null geodesic and that the observers worldline crosses the geodesic at the point of intersection between photon and observer. Hmmm. Yeah. That makes sense. Thanks MJ.

Pete
 
  • #17
MeJennifer said:
The sub-lightspeed particle that emits the photon is indeed spacelike related to the observer, however that is not the case for the emitted photon. On the plane of simultaneity you will notice that both the temporal distance and spatial distance between the emitted photon and the observer is zero.

I think you're either confused or using standard terms in nonstandard ways.

The terms "spacelike" or "timelike" or "lightlike"-related only refer to a pair-of-events, not a pair-of-observers (or a pair-of-observer-worldlines).

Here is a [Minkowski] spacetime diagram of the situation you describe:
[tex]
\]
\begin{picture}(200,200)(0,0)
\unitlength 2mm
{
\qbezier(0,50)(0,0)(0,0)\put(0,0){O}
\qbezier(0,0)(60,0)(60,0)\put(0,50){T}
}
{
\put(30,50){S}
\qbezier(30,50)(40,0)(40,0)
\qbezier(00,10)(40,0)(40,0)
\put(0,10){F}
}
{
\put(40,0){E}
\qbezier(40,0)(0,40)(0,40)
\put(0,40){R}
}
{
\qbezier(0,0)(40,40)(40,40)
\put(33,33){P}
\put(20,20){X}
}
\end{picture}
\[
[/tex]

ES is the [timelike] worldline of the sub-lightspeed particle (the source)
EF is that particle's [spacelike] plane of simultaneity [which is Minkowski-orthogonal to ES]

OT is the [timelike] worldline of the observer (the receiver/absorber)
OE is the observer's [spacelike] plane of simultaneity [which is Minkowski-orthogonal to OT]

E is the emission event by the source
R is the reception/absorption event by the observer
ER is a lightlike spacetime path. In fact, ER is on the past-light-cone of event R.

Note that E and R are not simultaneous for the observer OT or the particle ES.
In fact, since E and R are lightlike-related, E and R cannot be spacelike-related, and thus cannot be simultaneous events for any timelike observer. That is why I commented on your earlier statements:
robphy said:
MeJennifer said:
But note that as soon as a photon was emitted in the direction of the observer then in the observer's frame of reference, using Einstein synchronized clocks, it has already been absorbed.

Are you saying that the target observer determines the emission event to be simultaneous [i.e. assigns the same time coordinate t (in accordance with his wristwatch)] with the absorption event?

MeJennifer said:
If we assume the observer uses Einstein clock synchronization then the answer is yes. Both the emission and the absorption of the photon are on the observer's plane of simultaneity.
Now let's parse your more recent post:
MeJennifer said:
The sub-lightspeed particle that emits the photon is indeed spacelike related to the observer
As I said above, spacelike-related only refers to pairs-of-events, not pairs-of-worldlines. While O-and-E and F-and-E are spacelike-related pairs of events (one on each worldline), O-and-P and E-and-R are lightlike-related and O-and-S and E-and-T are timelike-related.
MeJennifer said:
however that is not the case for the emitted photon.
Here, one can say that every event on the photon's spacetime path ER is lightlike-related to event R on the observer's worldline. However, note that the events on the segment XR are timelike-related to O on the observer's worldline, and the events on the segment EX are spacelike-related to O.

So, in summary, it is incorrect to use the term "spacelike-related" with anything but pairs-of-events.

MeJennifer said:
On the plane of simultaneity you will notice that both the temporal distance and spatial distance between the emitted photon and the observer is zero.

For the OT observer, the planes parallel to OE are his [spacelike] planes of simultaneity.
For each event Y on ER excluding event-R itself, the OT-observer determines the spatial-distance between event-Y and his worldline OT to be nonzero.

The only way I can see to make a true statement with a subset of your words is this... paraphrasing... The distance-between-these-two-lines OT and ER is zero since they intersect. But that will be true of any two intersecting lines, regardless of the nature of their tangent vectors.
 
  • #18
Robphy, any particular reason the line is sloped with respect to OT.
Let's make it a bit simpler, assume that OT and EF are at relative rest with each other.

So let's for the sake of argument assume that you are right and that the emission and absorption of the photon do not happen at the same time:

So let's clock synchronize, using the Einstein clock synchronization method OT frame.
Suppose E is emitted at 10:20 in the morning at what time is it absorbed at R?

With regards to the distance between the approaching photon and the event of absorbtion:

Pick any point you like on the photon's worldline and call it point A.
Then take the point where the photon and the wordline of the observer crosses and call this B.

Now calculate the distance between point A and B.

The distance between those two points is zero, under all circumstances!

:smile:
 
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  • #19
MeJennifer said:
Robphy, it is really very simple and straightforward:

Pick any point you like on the photon's worldline and call it point A.
Then take the point where the photon and the wordline of the observer crosses and call this B.

Now calculate the distance between point A and B.

The distance between those two points is zero, under all circumstances!

:smile:

Yes, I agree that the spacetime interval is zero between those two events A and B. Great job.

But many of the other comments that you made in this thread made little sense... using the standard terminology of special relativity and Minkowski spacetime. In particular, this makes no sense using standard terms:
MeJennifer said:
Both the emission and the absorption of the photon are on the observer's plane of simultaneity.
That quoted statement is simply false. I offered a correction to replace "observer's plane of simultaneity" with "the past light cone of the absorption event".
 
  • #20
So then answer what the time difference is between the emittance and absorption of the photon for an Einstein clock synchronized frame of reference.
I say it is zero, what do you say?

Let's take a "practical" example, say we put clocks everywhere between us and some object X which is 5 light hours away from us, which, for symplicity's sake, is at rest relative to us.
We synchronize all clocks using Einstein's method.
Then say at 10:30 in the morning we emit a photon in the direction of the object X. What will be the time, on the local clock near the object, when the photon is absorbed?
 
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  • #21
MJ - I posted a few questions for you in my last post in this thread. However you never answered the questions. Perhaps you thought that they were rehtorical? Let it be known that they were not rehtorical questions. I made some assumptions about what you seemed to be trying to say. Those assumptions were made so that I might arrive at the same conclusion that you did. But how can I be sure of this if you don't answer??

Best regards

Pete
 
  • #22
pmb_phy said:
MJ - I posted a few questions for you in my last post in this thread. However you never answered the questions. Perhaps you thought that they were rehtorical? Let it be known that they were not rehtorical questions. I made some assumptions about what you seemed to be trying to say. Those assumptions were made so that I might arrive at the same conclusion that you did. But how can I be sure of this if you don't answer??
Sorry for that.

Ok, you asked me when I wrote:

MeJennifer said:
Because, conform the Minkowski metric, the length of the photon's wordline is always zero, so then it follows that the distance between each point on this line and the space-time event that constitutes the absorbtion must be zero as well.
what I mean by "conform the Minkowski metric".

Well, the metric of space-time is such that the distance between any two points on a lightlike worldline is always zero. This in contrast to for instance an Euclidean metric in Galilean space-time.

Then you wrote:

pmb_phy said:
So what you're saying is that the photon is on the null geodesic and that the observers worldline crosses the geodesic at the point of intersection between photon and observer.
Yes, and the distance between any point on the photon's worldline and the absorbtion event is zero.
 
  • #23
I seemed to have germinated a discussion (worth while of course) in a direction other than what I originally intended. I neglected to mention Special Relativity.

I asked this question because I wanted to find out how special relativity handles energy changes under the Relativistic Doppler effect. The energy has to come from somewhere or go somewhere yet all inertial frames of reference are equal, c is the same and different observers will measure the frequency of the photon and obtain different results according to their relative velocity with respect to the source.

If you want you could imagine scientist One emitting a stream of long wave radiation photons and scientist Two detecting these as high energy gamma rays due to the relativistic Doppler effect – a massive increase in energy. If you want to put in some form of independent collision to cause the gamma ray to form the electron positron pair; fine – go ahead. The question is essentially the same. In SR observers are supposed to have god like powers of observation so scientist One should be able to deduce that it is his original photon that has undergone the transformations.
 
  • #24
ramcg1 said:
I seemed to have germinated a discussion (worth while of course) in a direction other than what I originally intended. I neglected to mention Special Relativity.

I asked this question because I wanted to find out how special relativity handles energy changes under the Relativistic Doppler effect. The energy has to come from somewhere or go somewhere yet all inertial frames of reference are equal, c is the same and different observers will measure the frequency of the photon and obtain different results according to their relative velocity with respect to the source.

If you want you could imagine scientist One emitting a stream of long wave radiation photons and scientist Two detecting these as high energy gamma rays due to the relativistic Doppler effect – a massive increase in energy. If you want to put in some form of independent collision to cause the gamma ray to form the electron positron pair; fine – go ahead. The question is essentially the same. In SR observers are supposed to have god like powers of observation so scientist One should be able to deduce that it is his original photon that has undergone the transformations.

Special relativity handles energy much the same way that Newtonian physics does. (I'm going to avoid talking about how GR handles energy, it's unfortunately more complex). But the case you are talking about is very simple and very similar to Newtonian theory.

In any given inertial frame, the total energy of an isolated system is a constant.

However, this does not imply that a "boost" transformation (a transformation from one inertial frame to a different inertial frame that's moving relative to the intitial frame) does not change the energy of a system.

In fact, it should be obvious that even in Newtonian physics, a "boost" of a system changes its energy. If you have a baseball that is standing still, if you perform a "boost" transformation to a different frame, the baseball now has kinetic energy - energy that it did not have before.

However, this energy did not "come from" anywhere. The energy of a system depends on the frame of reference used to measure it.

Your question simply replaces the baseball with a gamma ray. Just as in the baseball case, the energy of an isolated system in any given inertial frame is a constant. Also as in the baseball case, when you perform a "boost" on the system, the energy of the system will not be the same as it was for the "unboosted" system.
 
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  • #25
"The energy of a system depends on the frame of reference used to measure it."

Are you implying that by changing the frame of reference you change the total energy of a system? How does tha tconserve energy.
 
  • #26
ramcg1 said:
"The energy of a system depends on the frame of reference used to measure it."

Are you implying that by changing the frame of reference you change the total energy of a system? How does tha tconserve energy.
You have to take energy and momentum together in order to create a Lorentz invariant propery.
 
  • #27
ramcg1 said:
Are you implying that by changing the frame of reference you change the total energy of a system? How does tha tconserve energy.
The phrase conservation of energy refers to the fact that the sum of all energies of free particles does not depend on time. It does not mean that this energy won't change when the frame of reference changes.

Pete
 
  • #28
pmb_phy said:
The phrase conservation of energy refers to the fact that the sum of all energies of free particles does not depend on time. It does not mean that this energy won't change when the frame of reference changes.

Pete

Yep. Exactly what I was trying to say in my post.
 
  • #29
“You have to take energy and momentum together in order to create a Lorentz invariant propery.”

So in one frame of reference it has low energy and low momentum and in the other it has high energy and high momentum, but the velocity is c. Applying the transformation is mathematically acceptable but it still does not explain the energy increase. It is still the same photon.
 
  • #30
You are confusing the meanings of the words "conserved" and "invariant".

A conserved quantity remains the same as time passes, in the same inertial reference frame; but it may be different in different inertial reference frames.

An invariant quantity is the same in all inertial reference frames, but it may not be conserved in any particular inertial reference frame.

The energy of an object (whether a photon or some other kind of object) is conserved in any particular inertial reference frame, so long as it doesn't interact with something else, but it is not invariant between different inertial reference frames.
 
  • #31
OK, so it is not invariant, but it still still does not explain why the energy and momentum in one frame of reference is different to the energy and momentum in another frame of reference. If the object (whether a photon or some other kind of object) is in an intermediary position between the observers then it has two different energy levels at once. If the gamma ray interacts with an atomic nucleus how will Scientist One explain it?
 
  • #32
Let's be specific: a gamma ray is absorbed by a nucleus. The energy and momentum of the gamma ray is transferred to the nucleus, which recoils and also gains some internal energy.

The amount of energy lost from the gamma ray is the same as the total energy (internal + energy of motion) gained by the nucleus according to scientist 1, and according to scientist 2.

Note that scientist 1 and 2 do not have to agree on the total energy of the gamma ray + nucleus. In fact, they do not. What they do agree about is that the interaction between the gamma ray and the nucleus does not change the total energy of the system (but they don't agree on what the numerical value of that initial energy was).

Note that we've said essentially the same thing before, so please think about this a little bit.
 
  • #33
The two scientists agree that the atom has certain "internal" energy levels (-13.6 eV, -3.4 eV, etc. for a hydrogen atom). They disagree about the atom's overall translational kinetic energy, and its momentum, because these depend on the velocity of the atom, which in turn depends on the reference frame. Therefore, they disagree about the atom's total energy (internal + kinetic).

In a photon absorption or emission process, their disagreement about the atom's total energy exactly compensates for their disagreement about the photon's energy. They both agree that the total energy of the system before the absorption or emission equals the total energy afterwards, although they disagree on its amount.
 
  • #34
“Let's be specific: a gamma ray is absorbed by a nucleus. The energy and momentum of the gamma ray is transferred to the nucleus, which recoils and also gains some internal energy.

The amount of energy lost from the gamma ray is the same as the total energy (internal + energy of motion) gained by the nucleus according to scientist 1, and according to scientist 2.

Note that scientist 1 and 2 do not have to agree on the total energy of the gamma ray + nucleus. In fact, they do not. What they do agree about is that the interaction between the gamma ray and the nucleus does not change the total energy of the system (but they don't agree on what the numerical value of that initial energy was).”

So Scientist One could detect his Long Wave Photon with an aerial but Scientist Two needs a nucleus to absorb the gamma ray.
 
  • #35
Clarifying Einstein synchronisation

MeJennifer said:
So then answer what the time difference is between the emittance and absorption of the photon for an Einstein clock synchronized frame of reference.
I say it is zero, what do you say?

Let's take a "practical" example, say we put clocks everywhere between us and some object X which is 5 light hours away from us, which, for symplicity's sake, is at rest relative to us.
We synchronize all clocks using Einstein's method.
Then say at 10:30 in the morning we emit a photon in the direction of the object X. What will be the time, on the local clock near the object, when the photon is absorbed?
Simple. It will be 3:30 in the afternoon. Einstein synchronisation means that if a light signal is sent from A to B and instantly returned back to A then B's clock at the moment of reception/return is set to half way between A's emission time and reception time. So in practice B starts by setting his clock to zero when he receives/retransmits the signal and when A sends a later message to B indicating A's two times, B can advance his own clock by the average of A's two times. "Relativity of simultaneity" comes about simply because from another inertial frame with respect to which A and B are in colinear uniform motion at the same velocity, the moment of signal reflection at B does not occur halfway between A's emission and reception.

Furthermore, it is especially important to note that reciprocal time dilation also arises naturally from this difference in synchronisation and thus simultaneity, without the need for any difference in actual clock rates !
 
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FAQ: A scientist’s transmitter emits a wavelength

What is a scientist's transmitter?

A scientist's transmitter is a device that emits electromagnetic waves, also known as radio waves, at a specific wavelength. This wavelength is determined by the design and function of the transmitter.

How does a scientist's transmitter emit a wavelength?

A scientist's transmitter uses an antenna to convert electrical signals into electromagnetic waves. These waves are then transmitted through the air at a specific wavelength, which can be adjusted by the scientist.

What is the purpose of emitting a wavelength?

The purpose of emitting a wavelength is to send information or signals through the air. This can be used for various purposes such as communication, navigation, and scientific research.

What factors affect the wavelength emitted by a scientist's transmitter?

The wavelength emitted by a scientist's transmitter can be affected by factors such as the design of the antenna, the frequency of the electrical signals, and the surrounding environment. These factors can impact the strength and range of the transmitted wavelength.

How does a scientist determine the appropriate wavelength to emit?

The appropriate wavelength to emit depends on the intended purpose of the transmission. Scientists use various methods such as calculations, experiments, and simulations to determine the most effective wavelength for their specific needs.

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