From: ph@netcom.com (Peter Hendrickson)
To: ravage@bga.com
Message Hash: b8fcf9b1c9e4456bb9b0c69fad6b82febf948192e0c9ead1351dba10bd2c85b4
Message ID: <199403311657.IAA29961@mail.netcom.com>
Reply To: <199403311354.AA01893@zoom.bga.com>
UTC Datetime: 1994-03-31 16:49:20 UTC
Raw Date: Thu, 31 Mar 94 08:49:20 PST
From: ph@netcom.com (Peter Hendrickson)
Date: Thu, 31 Mar 94 08:49:20 PST
To: ravage@bga.com
Subject: Re: Bekenstein Bound (was: Crypto and new computing strategies)
In-Reply-To: <199403311354.AA01893@zoom.bga.com>
Message-ID: <199403311657.IAA29961@mail.netcom.com>
MIME-Version: 1.0
Content-Type: text/plain
Jim Choate writes:
>>
>> The Deutsch paper I quoted before was where I first heard of the Bekenstein
>> Bound which Eric Hughes mentioned. According to Deutsch:
>>
>> "If the theory of the thermodynamics of black holes is trustworthy, no
>> system enclosed by a surface with an appropriately defined area A can have
>> more than a finite number ...
> The problem I see with this is that there is no connection between a
> black holes mass and surface area (it doesn't have one). In
> reference to the 'A' in the above, is it the event horizon? A funny
> thing about black holes is that as the mass increases the event
> horizon gets larger not smaller (ie gravitational contraction).
If I read the quote correctly, the surface area of the black hole
itself is not under discussion. Rather, whether it can be contained
in a surface with some area, which it can be.
Peter
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