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Suppose one had some sort of mirror right near the event horizon at a fixed distance (ignoring the problems with a hugely tough tether to hold it up and so forth) and you tried to measure the near horizon physics of particle approaching the BH by their reflection. The elongation of transverse modes would mean a huge increase in the uncertainty in the position of the string, which creates this fuzziness. The mirror can only be held up to the limit of the stretched horizon. A string length above the GR horizon, and the only thing you could observe is their shortest transverse modes for gravity near the Planck scale--- everything else would be so uncertain that their positions are unobservable. Now if you decided to stand on that mirror to get a direct view you would find that the temperature of the vacuum region there would be horrendous. This has a curious duality of sorts with the more distant observation. The distant observer has set up a situation where the states of the vacuum near the mirror are observed in a squeezed state which increases the uncertainty in their transverse positions. The observer near the horizon or on this mirror observes a thermal hot bath. In both cases there is something analogous to the von Neumann entropy with a measurement.
The string tension is determined by the string coupling parameter α' as T = 1/2πα' and generalizes the uncertainty principle as
Δx ~ ħ/Δp α'p/ħ.
This is a form of T-duality as well where p is replaced by the radius of compactification or for p ~ 1/R. The uncertainty in length is then large (small) if α' is large (small), and the string tension is very small (large) correspondingly. If α' is very large then the string tension is small and the string can be stretched out enormously. This is similar to QCD at high energy where quarks are in a state of asymptotic freedom. Equivalently the uncertainty in the length of the string is large as well. This is a general sort of uncertainty principle
ΔxΔp ~ ħ α'pΔp /ħ,
and if we write Δp = Fδt so that
Fδx ~ ħc/δx α'pF/ħ .
Now we perform a summation over elements of δx_i and get
Σ_i F_iδx_i ~ ħc/δx^N Σ_i α'pF_i/ħ.
This is the scale of a fluctuation with an imaginary time τ = ħ/E, E = Σ_i F_iδx_i and E = kT. The temperature here is then an effective temperature corresponding to the degree of "chaos" induced by quantum uncertainty. The first term ħc/δx^N ~ 0 for N large and we get an effective entropy
kT ~ Σ_i α'pF_i/ħ.
So for the distant observer there is a Verlinde type of entropy or "entropy force of gravity," while for the close observer there is an enormous thermal bath of bosons (bosnoic strings etc) which manifests the same entropy.
Cheers LC