- #71
PeterDonis
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Tio Barnabe said:I thought ##d \tau^2## could always be regarded as a proper time, because in the reference frame of the "particle" there's no spatial displacement.
This will be true if the particle has nonzero rest mass and ##d\tau^2## is an interval along its worldline. But the definition of ##d\tau^2## makes no such assumptions. What you're describing is just one particular special case.
Tio Barnabe said:because if it is space-like the "proper time" would be negative?
The square root of ##d\tau^2##, assuming you were using a timelike signature convention, would not be negative for a spacelike interval, it would be imaginary.
However, this is still focusing on superficial features instead of the fundamental definition. The fundamental definition just says that timelike, null, and spacelike intervals are physically different. How that difference is modeled in the math depends on your choice of signature convention--note that I specified a timelike signature convention above, which means that timelike intervals have positive ##d\tau^2## and spacelike intervals have negative ##d\tau^2##. Conversely, the spacelike signature convention means that timelike intervals have negative ##d\tau^2## (the symbol ##ds^2## is normally used in this case--but as I said before, it's often used in the timelike signature case as well) and spacelike intervals have positive ##d\tau^2##. Either way, null intervals have zero ##d\tau^2##.