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Equation 68 · Part 1 · The Bit Comes Back Before the Bearing

Symbol t_*

t∗≈3.5 mst_* \approx 3.5\,\mathrm{ms}
t∗t_*

What this part means

t∗t_* is a part of this expression. Its role is fixed by the surrounding article and by the operations shown in the formula.

Its job in the formula

t∗t_* is a part of this expression. Its role is fixed by the surrounding article and by the operations shown in the formula.

The passage around this formula

where the second equality for a Schwarzschild hole 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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Sources cited in the surrounding passage

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