On Wednesday, January 22, 2020 at 9:03:55 PM UTC-7, Alan Grayson wrote:
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>
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> On Wednesday, January 22, 2020 at 8:54:37 PM UTC-7, Brent wrote:
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>>
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>> On 1/22/2020 6:38 PM, Alan Grayson wrote:
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>> On Wednesday, January 22, 2020 at 1:34:00 PM UTC-7, Lawrence Crowell 
>> wrote: 
>>>
>>> On Wednesday, January 22, 2020 at 11:33:04 AM UTC-6, John Clark wrote: 
>>>>
>>>> On Wed, Jan 22, 2020 at 12:06 PM Lawrence Crowell <
>>>> [email protected]> wrote:
>>>>
>>>> > *It is then possible to have an expanding accelerated cosmos that is 
>>>>> spherically closed.*
>>>>
>>>>
>>>> So if I keep going I will eventually return to where I started even 
>>>> though everything is constantly getting more distant from me and is doing 
>>>> so at an accelerating rate?
>>>>
>>>>  John K Clark
>>>>
>>>
>>> For an accelerated expansion of the sphere there is a cosmological 
>>> horizon that one can't cross. in other words, the sphere will keep 
>>> expanding faster than you can ever go. Think of the scene in the movie 
>>> "*The 
>>> Shining*" with Jack Nicholson where the hotel hallway telescoped away 
>>> faster than he could run.
>>>
>>> LC
>>>
>>
>> I don't think it depends on acceleration. As long as the universe 
>> expands, even at a constant rate, at some distance, the distance between, 
>> say, an Earth observer, and some terminal point along a line of sight, will 
>> exceed 300,000 km (the distance light travels in one second) and points 
>> beyond that will keep increasing the increment every second, creating a 
>> cosmological horizon that light cannot cross. 
>>
>>
>> That's not quite right.  Light can cross it just fine.  But a photon 
>> crossing it toward us, can never reach us.  This is how the Hubble boundary 
>> differs from a black hole event horizon.
>>
>> Brent
>>
>
> Good point. TY. AG 
>

Now I'm not so sure. ISTM, the photons that never reach us, never cross the 
event horizon. They're emitted in a region receding faster than the SoL, so 
they can never cross it. AG 

>
>> This is because the creation of the horizon is purely a geometric effect 
>> of the expansion, and the rate of expansion is irrelevant. AG
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