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

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