Early universe, hence no observers
If the low entropy fluctuation is of the form supposed by Sean Carroll - that is, it produces the conditions for cosmological inflation to occur, it will be irrelevant to any evolved observers who appear well after the early rapid inflation phase.
Immediately related elementsHow this works
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The Arrow of Time  »The Arrow of Time 
The physics of time »The physics of time
The thermodynamic arrow »The thermodynamic arrow
Why do we see an entropy gradient? »Why do we see an entropy gradient?
Asymmetric boundary condition »Asymmetric boundary condition
Past hypothesis »Past hypothesis
Why low entropy in the past? »Why low entropy in the past?
Anthropic selection »Anthropic selection
Low entropy generators »Low entropy generators
Source of low-entropy states »Source of low-entropy states
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Early universe, hence no observers
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