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 
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The physics of time »The physics of time
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The thermodynamic arrow »The thermodynamic arrow
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Why do we see an entropy gradient? »Why do we see an entropy gradient?
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Asymmetric boundary condition »Asymmetric boundary condition
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Past hypothesis »Past hypothesis
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Why low entropy in the past? »Why low entropy in the past?
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Anthropic selection »Anthropic selection
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Low entropy generators »Low entropy generators
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Source of low-entropy states »Source of low-entropy states
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Can observers see low entropy? »Can observers see low entropy?
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Early universe, hence no observers
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