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Equation 64 · Part 1 · The Bit Comes Back Before the Bearing

Symbol t_*

t∗  ∼  β2π ln⁡S,β≡ℏkBTH=8πGMc3,t_* \;\sim\; \frac{\beta}{2\pi}\,\ln S, \qquad \beta \equiv \frac{\hbar}{k_BT_H} = \frac{8\pi GM}{c^3},
t∗t_*

What this part means

t∗t_* is part of the quantity the equation computes from the expression on the right.

Its job in the formula

t∗t_* is part of the quantity the equation computes from the expression on the right.

The passage around this formula

…follows directly from Hawking’s temperature formula [ 7 ] and S = A/4ℓP2\ell_P^2 is the Bekenstein-Hawking entropy [ 6 ] . For a solar-mass hole, β\beta ≈\approx 1.24×\times10^{-4}\,s\mathrm s and ln⁡\ln S ≈\approx 177 , giving t∗t_* ≈\approx 3.5\,ms\mathrm{ms} — an exact evaluation of the stated formulas, illustrative of the scrambling scale and not a claim about any particular measured hole.

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A subscript is a label attached below a symbol. It often selects a time step, component, category, or member of a sequence.

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