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|    sci.physics    |    Physical laws, properties, etc.    |    178,769 messages    |
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|    Message 178,229 of 178,769    |
|    Paul B. Andersen to All    |
|    Re: What came first the stars or the ear    |
|    15 Sep 25 21:25:11    |
      XPost: sci.physics.relativity       From: relativity@paulba.no              Den 15.09.2025 08:38, skrev Thomas Heger:       >       > It starts with the lack of a proper definition of t_A and t_B.       >       > If disconnected local times are meant with 'A-time' and 'B-time' and t_A       > was measured in 'A-time' and t_B by means of 'B-time', than       > t_B-t_A would be an illegal operation to begin with.       >       > Therefore t_A and t_B must be based on 'A-time' only. And that in turn       > would make 'B-time' irrelevant.       >       > That isn't bad at all, because the clock in B shall be synchronized with       > the clock in A, anyhow.       >              quote from § 1. Definition of Simultaneity       -------------------------------------------       | "If at the point A of space there is a clock, an observer       | at A can determine the time values of events in the immediate       | proximity of A by finding the positions of the hands which       | are simultaneous with these events.       | If there is at the point B of space another clock in all       | respects resembling the one at A, it is possible for an observer       | at B to determine the time values of events in the immediate       | neighbourhood of B."              An observer at A can determine the time value of the clock at A.       An observer at B can determine the time value of the clock at B.       Got it?              quote from § 1. Definition of Simultaneity       -------------------------------------------       | "But it is not possible without further assumption to compare,       | in respect of time, an event at A with an event at B.       | We have so far defined only an “A time” and a “B time.”              It is not possible to compare the time of events at A and       the time of event at B without further assumptions.       Got it?              So we have to make further assumptions:              quote from § 1. Definition of Simultaneity       -------------------------------------------       | "We have not defined a common “time” for A and B, for       | the latter cannot be defined at all unless we establish       | by definition that the “time” required by light to travel       | from A to B equals the “time” it requires to travel from       | B to A."              The _definition_ of simultaneity is that light uses the same       time to go from A to B and to go from from B to A.       Got it?              quote from § 1. Definition of Simultaneity       -------------------------------------------       | "Let a ray of light start at the “A time” tA from A towards B,       | let it at the “B time” tB be reflected at B in the direction       | of A, and arrive again at A at the “A time” t′A."              tA, tB and t'A are precisely defined as:       tA is the time shown by the clock at A when the ray leave A.       tB is the time shown by the clock at B when the ray hits B.       t'A is the time shown by the clock at A when the reflected ray hits A.       Got it?              quote from § 1. Definition of Simultaneity       -------------------------------------------       | " In accordance with definition the two clocks synchronize if       | tB − tA = t′A − tB."              For this equation to be true must        tB = (tA + t′A)/2 = tA + (t'A - tA)/2              Note that Einstein says nothing about how to make       asynchronous clocks synchronous. He only says that       if tB − tA = t′A − tB (or TB = tA + (t'A - tA)/2)       then the clock at A and the clock at B are synchronous.       This is a definition of simultaneity, not a description       of how to synchronise clock.       --------              How to synchronise clocks depend on a lot of circumstances,       and it would be stupid of Einstein to define a method       which should be applicable for all cases in all future.              To illustrate this problem let's ask:       How do we synchronise TAI and UTC clocks?              Let two clocks A and B be stationary at the geoid at equator.       Clock B is a distance L east of clock A.       We know that clock A is synchronous with UTC, and we want to       synchronise clock B to UTC.              How do w do it?       The problem is that TAI and UTC clocks are synchronous in       the non rotating Earth centred frame of reference (ECI-frame),       they are NOT synchronous in the ground frame.       But the clocks A and B are moving in the ECI-frame, and       we can't stop the spinning of the Earth to sync the clocks.              The following calculations are made in the ECI frame.       v = 465.1 m/s v/c = 1.55e-6              We assume that at t = 0 the clocks are synonymous and show 0.       That is at t = 0, tA = 0 and TB = 0.       If we send a light pulse from clock A to clock B, clock B       will move away from clock at the speed v.       We can calculate the time the light pulse will use to hit B:        ct = L + vt => t = L/(c-v) = (L/c)⋅(1 + 1.55e-6)              That means that if clock A showed t1 when the light pulse       was emitted, then, to be synchronous with clock A, clock B       must show t1 + (L/c)⋅(1 + 1.55e-6) when the pulse hits it.              TAI clocks are routinely synced after the basic principle shown above.       (The details are different of course. Satellites, optic fibre, radio)              --       Paul              https://paulba.no/              --- SoupGate-Win32 v1.05        * Origin: you cannot sedate... all the things you hate (1:229/2)    |
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