Exploring Time Dilation and the Lawrentz Factor

In summary, the conversation discusses the concept of time dilation in special relativity and the use of the Lorentz factor in determining it. The conversation also brings up a potential flaw in the commonly reduced equation for the Lorentz factor and its application in vector problems. The comparison is made to the Doppler effect and the importance of not using cancellation incorrectly in equations. The conversation ends with a disagreement over whether or not there is a flaw and the importance of understanding the use of vectors and equations in physics.
  • #1
A(s)
58
0
First off I apologize for lengthiness, but I want to be thorough... please read the entire postI was just reading up on time dilation on wiki, and saw that the formula for determining time dilation in special relativity is essentially delta t times the Lawrentz factor.

in other words for time dilation,

t / [(1 - v^2 / c^2)^1/2]

The lawrentz factor describes things like time dilation, length contraction and relative mass, but I think there may be a problem with the application of it. The lawrentz factor is

c / [(c^2 - v^2)^1/2]

but it is commonly reduced to

1 / [(1 - B^2)^1/2]

where B = v / c

this reduction is done by simply pulling out a c^2 from under the square root, and then canceling it with the top c.

Here is the problem.If we are dealing with a vector problem, as most time dilation theories do, (i.e. traveling out at a significant fraction of the speed of light, and coming back at the same speed therefore reducing the aging process) the reduced equation essentially assumes absolute values of the vectors. Here is an example.
NO ASSUMPTIONS PLEASE KEEP READING
Let us assume for the problem a reference point of (0,0,0) coordinates in space on an X,Y,Z axis.

The direction we will travel from point (0,0,0) to planet A will be in a positive Z direction at a rate of 2.0E8 meters per second with no X or Y components. Assume the distance is such that it takes 5 days on a spacecraft to get there.

Using the unreduced formula, the Lawrentz factor for the trip there will be

3.0E8 / [((9.0E16)-(4.0E16))^1/2] = 3.0E8 / 2.24E8 = 1.34

on the trip back we have

-3.0E8 / [((9.0E16)-(4.0E16))^1/2] = -3.0E8 / 2.24E8 = -1.34

the -3.08 on top must be negative because the speed of light and the velocity we determined are relative to a positive z vector, but now we are headed in a negative z direction... so a factor describing relative time and speed to a stationary point must maintain that relativity. The -3.0E8 and -2.0E8 on the bottom were both squared according to the equation, and thus lost the signs attributed to them, leaving them at 9.0E16 and 4.0E16 (i know this is basic, but i must point it out to avoid argument)

if we add the lawrentz factors, the total difference in relative time is 0

5days(1.34) +5days(-1.34) = 0

Finally, If we did this same equation with the reduced formula (where c had been canceled out), we would get 1.7 days fewer on both the trip there and the trip back, leaving us 3.4 days "younger" than our brothers at point (0,0,0)

How has nobody noticed this flaw...To me, this is similar to the Doppler effect. If you hear an ambulance going away from you the pitch decreases. When it comes closer to you the pitch increasesIf you had a telescope and you were able to watch the spaceship fly away from point (0,0,0) it would take you 1.7 days to observe 1 day of behavior on the ship... the light is stretched out... but if you watch the way back, it will only take you about .746 days to observe one day of behavior, because the light would be compacted and closer together... regardless, the entire trip could be observed in exactly 10 days. It would just appear to take 6.7 days for them to get there and 3.3 days for them to get back...can anyone echo if I am on to something here? and why it hasn't been noticed before?
 
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  • #2
First-off, it's "Lorentz". :smile:

A(s) said:
To me, this is exactly like the Doppler effect. If you hear an ambulance going away from you it sounds like it is getting quieter but it is not. When it comes close to you, it sounds like it is getting louder but it is not.

Careful - Doppler has to do with pitch, not amplitude. Amplitude does vary with distance, and pitch/frequency varies with relative velocity (i.e. approaching/receding).

Regards,

Bill
 
  • #3
well pitch is frequency, which is cycles per second,

light waves more cycles per second = more densely perceived time

same as higher pitch = more densely perceived sound

In sound this is shown in the crests and troughs being closer together or further apart at the same speed

with light this would be shown with photons being closer together or further apart at the same speed
 
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  • #4
A(s) said:
by faster i mean more cycles per second, not higher speed

I realize what you meant to say, but "quieter"/"louder" means something else.

Regards,

Bill
 
  • #5
thank you I will edit that
 
  • #6
A(s) said:
In sound this is shown in the crests and troughs being closer together or further apart at the same speed

with light this would be shown with photons being closer together or further apart at the same speed

Not exactly - what you said of sound would be true of light as well.

Regards,

Bill
 
  • #7
so it might move off the visible spectrum because frequency increases or decreases, but the photons would still be released closer together or further apart depending on the direction of travel
 
  • #8
A(s):
can anyone echo if I am on to something here? and why it hasn't been noticed before?
Is it maybe just possible that you're wrong ? This has been scrutinised for over 100 years and you'd think any problems of the kind you point out would have been found.
 
  • #9
Of course it is possible that I am wrong, but i would expect a better reason other than nobody else has realized it

if you have the equation of a line as y = (x^2 -1)/(x-1) even though it reduces to y = x+1 does not mean that they are the same line... one line has a hole or does not exist at x=1... the other exits at all values.

cancellation is a very dangerous thing if used incorrectly
 
  • #10
to apply my previous statement directly to this problem... Y = b/ (b^2)^(1/2) does not equal 1 if b is negative... it equals -1
 
  • #11
Come on: c stands for the speed of light; it's not a vector quantity.

The "Lorentz factor" is:

[tex]\gamma = \frac{1}{\sqrt{1 - v^2/c^2}}[/tex]
 
  • #12
A(s) said:
First off I apologize for lengthiness, but I want to be thorough... please read the entire postI was just reading up on time dilation on wiki, and saw that the formula for determining time dilation in special relativity is essentially delta t times the Lawrentz factor.

in other words for time dilation,

t / [(1 - v^2 / c^2)^1/2]

The lawrentz factor describes things like time dilation, length contraction and relative mass, but I think there may be a problem with the application of it. The lawrentz factor is

c / [(c^2 - v^2)^1/2]

but it is commonly reduced to

1 / [(1 - B^2)^1/2]

where B = v / c

this reduction is done by simply pulling out a c^2 from under the square root, and then canceling it with the top c.

Here is the problem.If we are dealing with a vector problem, as most time dilation theories do, (i.e. traveling out at a significant fraction of the speed of light, and coming back at the same speed therefore reducing the aging process) the reduced equation essentially assumes absolute values of the vectors. Here is an example.
You're not dealing with a vector problem. The "c" and "v" in those formulas are only meant to be speeds, i.e. v is just the absolute value of the velocity vector, and c is just a constant speed. If someone changes speeds, then if you want to calculate the time elapsed on their clock between two coordinate times [tex]t_0[/tex] and [tex]t_1[/tex], and their speed as a function of time in your chosen coordinate system is v(t), then the total elapsed time is [tex]\int_{t_0}^{t_1} \sqrt{1 - v(t)^2 / c^2} \, dt[/tex]
 
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  • #13
ok, well even still, if the relative direction of the speed of light has no bearing, what if you pull out v^2 out of the square root. the negative velocity might apply.

gamma = plus or minus c / [v(c^2 / v^2) -1)]if v is negative, you still get a negative value
 
  • #14
how are vectors irrelevant... with the doppler effect, you don't take absolute value and say that as a source of sound is approaching, the pitch decreases
 
  • #15
A(s) said:
how are vectors irrelevant... with the doppler effect, you don't take absolute value and say that as a source of sound is approaching, the pitch decreases
Time dilation is not based on the doppler effect, so how is this relevant? Clocks moving at the same speed are slowed down by the same factor, regardless of their direction.
 
  • #16
i suppose i am just wrong then... they seem really simmilar though
 
  • #17
A(s) said:
ok, well even still, if the relative direction of the speed of light has no bearing, what if you pull out v^2 out of the square root. the negative velocity might apply.

gamma = plus or minus c / [v(c^2 / v^2) -1)]if v is negative, you still get a negative value
Just think of v as the absolute magnitude of the velocity vector, which can't be negative.
 
  • #18
A(s) said:
so it might move off the visible spectrum because frequency increases or decreases, but the photons would still be released closer together or further apart depending on the direction of travel

The "visible spectrum" is a rather limited range of frequencies, but yeah - wavelengths could shift into/out of it via Doppler effects. Recall that one end of the spectrum is DC, while the other end is infinite frequency.

Whether the photons appear closer together or farther apart (relative to the frame in which they are emitted) depends upon the observer. If photons were produced at a certain rate within the frame of emission, they would be observed at a relative rate equivalent to the relative (proportional) change in wavelength (time dilation between frames).

Regards,

Bill
 
  • #19
Doc Al said:
The "Lorentz factor" is:

[tex]\gamma = \frac{1}{\sqrt{1 - v^2/c^2}}[/tex]

Let [itex]\frac{v}{c}=cos(\theta)[/itex] and then [itex]\theta=asin(\frac{1}{\gamma})[/itex].

Regards,

Bill
 
  • #20
Note that there is a relativistic version of the Doppler effect. It's derived similarly to the classical Doppler effect, but the effects of time dilation on the moving source are taken into account.

http://hyperphysics.phy-astr.gsu.edu/hbase/relativ/reldop2.html

The frequency that is received by the observer increase if the source is approaching, and decreases if the source is receding, just as with the classical Doppler effect, but the details are different.
 
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  • #21
jtbell said:
Note that there is a relativistic version of the Doppler effect. It's derived similarly to the classical Doppler effect, but the effects of time dilation on the moving source are taken into account.

http://hyperphysics.phy-astr.gsu.edu/hbase/relativ/reldop2.html

The frequency that is received by the observer increase if the source is approaching, and decreases if the source is receding, just as with the classical Doppler effect, but the details are different.

How does one get from the bi-directional classical version to the (Lorentz-consistent) unidirectional version without losing a sense of direction? Additionally, why does it appear that [itex]v_{wave}[/itex] changes to c in the process? .

Regards,

Bill
 
  • #22
Antenna Guy said:
How does one get from the bi-directional classical version to the (Lorentz-consistent) unidirectional version without losing a sense of direction?
The relativistic doppler shift equation is bidirectional too (you see a clock ticking faster than your own as it approaches you, and slower than your own as it moves away, slowed down by an amount even larger than the time dilation factor), it's only time dilation that doesn't depend on direction.
 
  • #23
On that page, for some reason they show the [itex]\pm[/itex] sign explicitly in the classical Doppler shift formula, but they hide it in the relativistic Doppler formula. In the classical formula, you substitute a positive number for the speed and choose either the + or - sign from the formula, but in the relativistic formula you substitute either a positive or negative number depending on the direction of motion.
 
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  • #24
A simple derivation of the relativistic Doppler effect follows from the fact that
[tex](\omega/c,\b{k})[/tex] is a four vector. Lorentz transformation gives
[tex]\omega'=\gamma\omega(1+v\cos\theta/c)[/tex], which includes a "transverse Doppler effect".
 
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  • #25
jtbell said:
Note that there is a relativistic version of the Doppler effect. It's derived similarly to the classical Doppler effect, but the effects of time dilation on the moving source are taken into account.

http://hyperphysics.phy-astr.gsu.edu/hbase/relativ/reldop2.html

The frequency that is received by the observer increase if the source is approaching, and decreases if the source is receding, just as with the classical Doppler effect, but the details are different.

that helps a bunch, thanks
 
  • #27
JesseM said:
The relativistic doppler shift equation is bidirectional too (you see a clock ticking faster than your own as it approaches you, and slower than your own as it moves away, slowed down by an amount even larger than the time dilation factor), it's only time dilation that doesn't depend on direction.

The URL claims that the sign of v (in the relativistic form) depends upon whether the source is moving toward or away from the observer - which inverts the [itex]v_{source}[/itex] coefficient, and does imply something in the way of a directional dependence. If I let r represent the distance to the source in some direction [itex]\hat{r}[/itex], and v be [itex]\frac{\delta r}{\delta t}[/itex], then the sign of v changes automatically to account for decreasing/increasing radial distance as a function of time.

Regards,

Bill
 
  • #28
Antenna Guy said:
The URL claims that the sign of v (in the relativistic form) depends upon whether the source is moving toward or away from the observer - which inverts the [itex]v_{source}[/itex] coefficient, and does imply something in the way of a directional dependence.
Yes, that's what I just said! The relativistic doppler effect does have a directional dependence, while time dilation does not.
 
  • #29
JesseM said:
Yes, that's what I just said! The relativistic doppler effect does have a directional dependence, while time dilation does not.

Now that we've cleared that up, what do you figure the answer to my question might be?

It's seems we agree (in an awkward sort of way) that the relativistic form is uni-directional; but the question of "why?" remains. The classical version yields two answers for one velocity (bi-directional result) - the relativistic form yields one answer for one velocity (uni-directional result).

Conceptually, I don't have any problem with negative velocities - It just struck me as odd to see a need for them within the context of SR.

Regards,

Bill
 
  • #30
You're free to write the relativistic equation with the plus/minus signs out in the open like this, to make it consistent with the non-relativistic one:

[tex]\nu_{observed} = \nu_{source} \sqrt{ \frac {1 \pm v/c}{1 \mp v/c}}[/tex]

In this form, v is always a positive number.
 
  • #31
Antenna Guy said:
It's seems we agree (in an awkward sort of way) that the relativistic form is uni-directional; but the question of "why?" remains. The classical version yields two answers for one velocity (bi-directional result) - the relativistic form yields one answer for one velocity (uni-directional result).
I guess I don't understand what you mean by "two answers for one velocity". Do you mean "speed" rather than "velocity"? In the classical version, two objects which have equal speeds along the axis from the viewer to the object but opposite velocities (i.e. opposite directions, one object coming towards the viewer and one moving away) yield different doppler shifts, and exactly the same thing is true in the relativistic version. I don't understand why you think they're different, except for the magnitude of the shift for a particular velocity.
 

1. What is time dilation?

Time dilation is a phenomenon in which time appears to pass slower for an object or observer that is moving at high speeds relative to another object or observer. This is due to the effects of special relativity and the Lawrentz factor.

2. How does the Lawrentz factor relate to time dilation?

The Lawrentz factor is a mathematical expression used to calculate the amount of time dilation that occurs for an object or observer moving at high speeds. It takes into account the velocity of the object and the speed of light.

3. What are some real-life examples of time dilation?

One of the most well-known examples of time dilation is the famous "twin paradox", in which one twin travels at high speeds in a spaceship while the other stays on Earth. When the traveling twin returns, they will have aged less than the twin who stayed on Earth. Other examples include the time dilation experienced by astronauts in space and the GPS system, which must account for time dilation in order to function accurately.

4. Can time dilation be observed or measured?

Yes, time dilation has been observed and measured in various experiments and real-life scenarios. One example is the famous Hafele-Keating experiment in which atomic clocks were flown on airplanes at high speeds, and their time readings were compared to clocks that remained on the ground. The clocks on the airplanes were found to have experienced time dilation.

5. How does time dilation impact our daily lives?

Time dilation may seem like a concept that only applies to extreme scenarios, such as space travel, but it actually has an impact on our daily lives. GPS systems, for example, must account for time dilation in order to function accurately. Additionally, the effects of time dilation can be observed in our everyday lives, such as the difference in aging between someone who travels frequently at high speeds and someone who does not.

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