Time with no gravitational force

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Discussion Overview

The discussion revolves around the theoretical implications of time in a region devoid of gravitational mass, exploring concepts of time dilation and the nature of spacetime. Participants examine the effects of gravity on the passage of time and question the behavior of light in such hypothetical scenarios.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions the assertion that time would not pass at all in a massless region, referencing equations related to proper time and spacetime intervals.
  • Another participant confirms that time does pass slower near the Sun compared to the Earth, but notes that the difference is minimal outside extreme gravitational fields.
  • A participant expresses uncertainty about how time would behave in a massless region, indicating a lack of clarity on the topic.
  • One participant suggests that time would pass extremely fast in a gravity-free spacetime, but acknowledges the ambiguity of this statement.
  • Another participant elaborates on the concept of temporal velocity and its relation to gravitational fields, emphasizing that in flat spacetime, the rate of time passage is similar to everyday experiences.
  • A later reply clarifies that flat spacetime is still considered a gravitational field and discusses solutions to Einstein's field equations in the absence of mass.

Areas of Agreement / Disagreement

Participants generally agree that time passes slower in stronger gravitational fields, such as near the Sun, but there is no consensus on the behavior of time in a hypothetical massless region. Multiple competing views and uncertainties remain regarding the implications of such a scenario.

Contextual Notes

There are unresolved questions regarding the assumptions made about spacetime without mass, the definitions of time passage in such contexts, and the implications for light travel in these regions.

Guiga
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Hello everyone,

I was doing my Physics homework and a question arose from it: if a mass affects time there is a difference in the time measured near different masses. However if there was no mass at all?
Let's pretend this is possible just for theoretical purposes, a perfectly flat space-time. In this situation time would not pass at all.
So how can light travel through such regions? (I know there is not such a thing in the Universe but intergalactical space may have very little space-time distortion.)

Just to confirm if my understanding is correct: time would pass slower near the Sun than near the Earth? (imagine they are both static, they do not have either translation or rotation)

Thank you very much!
 
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Why do you say time will not pass at all? ds^{2} = -dt^{2} + dx^{2} + dy^{2} + dz^{2} and \tau = \int_{\gamma }(-g_{\mu \nu }dx^{\mu }dx^{\nu })^{1/2} so in the rest frame of a test particle \Delta \tau = \int_{t_{i}}^{t_{f}}dt = \Delta t so there is a passage of proper time.
 
1. This should go in the Homework section.
2. Yes, time does pass slower near the Sun than near the Earth(however, both amounts of time dilation are so small they are irrelevant, we aren't near neutron stars or black holes here)

I really do not know how time would pass in such a region. That is really beyond me. There are plenty of people here who know more about this stuff than I do.
 
Hi WannabeNewton,

I couldn't understand perfectly the equation you posted but I got the idea. So actually my reasoning was misleading, time would be pass extremely fast in a space-time without gravity.
Is this difference in time taken into account when calculating distances in light-years?

xeryx35, this question was not from my homework, actually the way I wrote made it confusing.

Thanks!
 
When you say extremely fast, it's somewhat meaningless. Anyone can travel through time, its given by your temporal velocity which comes from the velocity 4-vector, u_{\alpha}=\langle u_0, \vec{u} \rangle. Here we can look at u_0, which equals u_0=\gamma c=\frac{c}{\sqrt{1-\frac{v^2}{c^2}}} where v^2 is the magnitude of the 3-velocity. This can also be written
<br /> \gamma=\frac{1}{\sqrt{1-\frac{v^2}{c^2}}}=\frac{dt}{d\tau}<br />
where \tau is the proper time. This says you can move through time at a maximum speed of 1 sec/sec, which is essentially what you are experiencing now relative to the rest of us and everyday experiences. But as you seemed to have picked up, this depends on the gravitational field one is immersed in, so in flat space, you are moving through time at essentially the rate you are moving through it right now since the curvature is practically negligible.
 
Flat spacetime is a gravitational field. its commonly expressed as \eta_{\alpha\beta}. In Einstein's relativity, there are sill solutions to the field equations that determine the dynamics of gravity even in the absence of sources of gravitation. This is similar to Maxwell's equations, for instance \vec{\nabla}\cdot\vec{E}=\rho /\epsilon_0 still has solutions even when \rho=0, that is, there are "free-field solutions". In fact there are many solutions that satisfy the vacuum equations, for instance, the solution describing the spacetime around our star, Sun. I hope this puts some things in order for you.
 

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