On 11/7/2019 10:42 PM, Alan Grayson wrote:


On Thursday, November 7, 2019 at 10:54:33 PM UTC-7, Brent wrote:



    On 11/7/2019 8:43 PM, Alan Grayson wrote:


    On Thursday, November 7, 2019 at 5:20:13 PM UTC-7, Brent wrote:



        On 11/7/2019 4:06 PM, Alan Grayson wrote:


        On Thursday, November 7, 2019 at 11:41:11 AM UTC-7, Brent
        wrote:


            On 11/6/2019 10:31 PM, Alan Grayson wrote:
            On Wednesday, November 6, 2019 at 11:20:23 PM UTC-7,
            Brent wrote:


                On 11/6/2019 9:00 PM, Alan Grayson wrote:

                On Wednesday, November 6, 2019 at 7:17:21 PM
                UTC-7, Brent wrote:



                    On 11/6/2019 4:44 PM, Alan Grayson wrote:


                    On Wednesday, November 6, 2019 at 3:46:54 PM
                    UTC-7, Brent wrote:



                        On 11/6/2019 12:05 AM, Alan Grayson wrote:


                        On Tuesday, November 5, 2019 at 10:23:58
                        PM UTC-7, Brent wrote:



                            On 11/5/2019 9:09 PM, Alan Grayson
                            wrote:

                                Crossing the horizon is a
                                nonevent for the most part. If
                                you try to accelerate so you
                                hover just above it the time
                                dilation and that you are in an
                                extreme Rindler wedge will mean
                                you are subjected to a torrent
                                of radiation. In principle a
                                probe could accelerate to
                                10^{53}m/s^2 and hover a Planck
                                unit distance above the
                                horizon. You would be at the
                                stretched horizon. This would
                                be almost a sort of singular
                                event. On the other hand if you
                                fall on an inertial frame
                                inwards there is nothing
                                unusual at the horizon.

                                LC


                            Do you mean that clock rates
                            continue to slow as an observer
                            approaches the event horizon; then
                            the clock stops when crossing, or
                            on the event horizon; and after
                            crossing the clock resumes its
                            forward rate? AG

                            He means the infalling clock doesn't
                            slow down at all. Whenever you see
                            the word "clock" in a discussion of
                            relativity it refers to an /*ideal
                            clock*/. It runs perfectly and never
                            speeds up or slows down.  It's
                            called /*relativity*/ theory because
                            observers /*moving relative*/ to the
                            clock /*measure it*/ to run slower
                            or faster than their (ideal) clock.

                            Brent


                        I see. So if for the infalling observer,
                        his clock seems to be running
                        "normally", but for some stationary
                        observer, say above the event horizon,
                        the infalling clock appears to running
                        progressively slower as it falls below
                        the EH, even if it can't be observed or
                        measured. According to GR, is there any
                        depth below the event horizon where the
                        infalling clock theoretically stops?

                        I just explained that */clocks never
                        slow/* in relativity examples.  So now
                        you ask if there's a place they stop??

                        Brent


                    I know, but that's not what I asked. Again,
                    the infalling clock is measured as running
                    slower than a stationary clock above the EH.
                    As the infalling clock goes deeper into the
                    BH, won't its theoretical rate continue to
                    decrease as compared to the reference clock
                    above the EH? How slow can it get? AG

                    It /*appears*/ (if the observer at infinity
                    could see the extreme red shift) to
                    /*asymptotically approach stopped */as it
                    approaches the event horizon.  This is because
                    the photons take longer and longer to climb
                    out because they have to traverse more and
                    more spacetime.

                    Brent


                I'm referring to two clocks; one at finite
                distance above the EH, and other infalling.
                Doesn't the infalling clock seem to run
                progressively slower from the POV of the other
                clock, as it falls lower and lower? AG

                I appears to run slower as seen by the distant
                observer.

                Brent


            As it goes deeper and deeper into the BH, does the
            clock ever appear to STOP? AG

            It doesn't appear at all when it passes the event
            horizon.  It appears to stop as it approaches the event
            horizon.

            Brent


        I know it can't be observed as it falls through the EH.
        That's why I referred to clock "readings" after falling
        through as "theoretical".

        Well it doesn't make much sense to call observations
        theoretical when it's the theory that says they can't be
        observed.

        On the other hand, LC says falling through the EH is a
        non-event, as if the infalling clock behaves as we expect
        based on a clock entering a region of strong gravitational
        field. But let's say the clock appears to stop as it
        approaches the EH, which is what I thought. How do you
        reconcile this prediction, which is certainly weird? AG

        Reconcile it with what?  It's a consequence of the metric
        which is derived from Einstein's equations. It's not as if
        it's some unexplained observation. It's not an observation at
        all.  It's a theoretical prediction.

        Brent


    You don't see a problem with a theory that predicts a clock which
    stops as seen by an outside observer, when the observer using the
    clock, which measures proper time, must see it moving forward?  AG

    No.  Why should it be a problem?  You're watching the clock
    approach the event horizon and the photons from it come further
    and further apart until you have to wait seconds between photons,
    and then hours, and then days, and years...why because they have
    to travel thru more spacetime.  If it's a rotating black hole, as
    most of them will be, each photon will have to orbit many times on
    it's way out.

    Brent


If clock which is fixed some distance from the EH, and the BH isn't rotating, why must the photons traveling to the fixed observer have to travel progressively longer times? AG

It's because there is more time to traverse.  It's a matter of the metric.

Brent

--
You received this message because you are subscribed to the Google Groups 
"Everything List" group.
To unsubscribe from this group and stop receiving emails from it, send an email 
to [email protected].
To view this discussion on the web visit 
https://groups.google.com/d/msgid/everything-list/bbe19a7b-11b7-5410-0d66-f9dbf30f0898%40verizon.net.

Reply via email to