On Mon, Oct 19, 2020 at 3:31 PM Jason Resch <[email protected]> wrote:

> On Sun, Oct 18, 2020, 10:33 PM Bruce Kellett <[email protected]>
> wrote:
>
>> On Mon, Oct 19, 2020 at 1:09 PM Jason Resch <[email protected]> wrote:
>>
>>> On Sun, Oct 18, 2020, 8:47 PM Bruce Kellett <[email protected]>
>>> wrote:
>>>
>>>>
>>>> Remember that entropy is basically related to the volume of phase
>>>> space, not of ordinary space. And phase space relates to the number of
>>>> particles (hence mass-energy). Spatial volume is essentially irrelevant for
>>>> volumes greater than that of the corresponding black hole.
>>>>
>>>
>>> No. Consider an infinite length. With a single atom you can encode
>>> infinite information through placement of the atom along that length.  This
>>> is with finite mass energy, but unrestricted spatial volume.
>>>
>>
>> That does not encode infinite information. There is, after all, only one
>> particle, and it can have only one position. If you want to encode more
>> information, you need more particles. You might need an infinite number of
>> bits to encode the position of one particle as a real number, but the
>> single particle cannot encode this.
>>
>
> This is plainly false.  Every 1 mile distance that particle is placed
> along the line encodes a unique number. Travel up to 2^N miles and you can
> encode N bits. With infinite range there's no upper bound.
>

A single particle can be in only one place, and encode on ly one bit.

> Or think of a grid of naughts and crosses, with a larger grid but fixed
> number of crosses, the number of possible combinations for drawing a fixed
> number of crosses still increases with more spaces to place them.
>

Each combination encodes only one combination.

An arbitrary volume can only hold a limited amount of energy, or entropy,
>> as given by the Bekenstein bound.
>>
>
> Energy isn't the same thing as entropy.
>

Bekenstein relates them.

> But the maximum entropy for a particular mass is given when that mass
>> forms a black hole -- which saturates the Bekenstein bound.
>>
>
> The bound is always satisfied. Black holes just reach the maximum of the
> bound at a given VOLUME.
>

I said saturated, not 'satisfied'. The bound gives the maximum possible
enclosed mass for a given volume, or the volume is that for which entropy
is maximum for a given mass which saturates the bound.

>
> Increasing the volume does not increase the actual entropy unless you
>> simultaneously increase the mass.
>>
>
> You keep saying this but don't provide any justification or sources. I
> implore you to read the wikipedia article and if it is wrong, please point
> me to a source with the right/corrected equation.
>

The justification is that it is impossible to increase the mass of a black
hole without at the same time increasing its radius (volume). For a black
hole, the radius is 2M, in natural units. So the mass and radius are
directly related. Any greater volume for the same mass does not saturate
the bound.



> As explained on that page, the bound is not limited to black holes, it
> says something more general which relates entropy bounds to the product of
> spherical radius and mass.
>

The entropy bound you are talking about is

   S <= 2pi RE.

This is saturated when the radius and energy are related as for a black
hole:

   R = 2M, for which S = 4pi M^2.

Nothing mysterious here. I was talking about maximum possible entropy,
which occurs when the bound is saturated, as for a black hole.

That is really all that the Bekenstein bound says. It is a bound, after
all, and has information about the entropy only when that bound is
saturated.

So for a fixed amount of mass, the entropy is maximized when that mass is
in the form of a black hole. Increasing the volume surrounding the BH makes
no difference to the entropy maximum for that mass.

Bruce

Jason
>
> In terms of the cosmological problem, the initial state has a particular
>> total mass, and that does not increase with the expansion of the universe.
>> Consequently, the maximum possible entropy does not increase either. The
>> point of the Past Hypothesis is that the initial state of this mass was of
>> low entropy since the gravitational degrees of freedom were not saturated
>> (it did not form a black hole), so there is a large amount of room
>> available for the entropy to increase.
>>
>> Bruce
>>
>

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