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τβ−≫τn(r-process)\tau_{\beta^-} \gg \tau_n \qquad \text{(r-process)}

Why this formula appears here

The rapid neutron-capture process runs the opposite calculation. Where the s-process waits for each nucleus to settle before moving on, the r-process floods a small volume of matter with so many free neutrons that a nucleus can capture several before it has any real chance to beta-decay: τβ−≫τn(r-process)\tau_{\beta^-} \gg \tau_n \qquad \text{(r-process)}. Under these conditions the reaction path runs far from the valley of stability, out toward the neutron drip line, where nuclei are so neutron-rich that adding one more neutron barely binds at all [ 8 ] . Capture continues, isotope after isotope, until it reaches a nucleus at one of the neutron shell closures — the magic neutron numbers 50, 82 and 126 — where the next capture is…

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τβ−\tau_{\beta^-}

Symbol tau_β^-

tau_β^- is a part of this expression. Its role is fixed by the surrounding article and by the operations shown in the formula.

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τn\tau_n

Symbol tau_n

taunu_n is a part of this expression. Its role is fixed by the surrounding article and by the operations shown in the formula.

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Published contexts (1)

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τβ−≫τn(r-process)\tau_{\beta^-} \gg \tau_n \qquad \text{(r-process)}

Equation 4 · Evolutionary Nuclear Physics

Nucleosynthesis Is Descent With Modification

This mathematical expression combines the displayed quantities; its precise role follows from the surrounding article text.

The rapid neutron-capture process runs the opposite calculation. Where the s-process waits for each nucleus to settle before moving on, the r-process floods a small volume of matter with so many free neutrons that a nucleus can capture several before it has any real chance to beta-decay: τβ−≫τn(r-process)\tau_{\beta^-} \gg \tau_n \qquad \text{(r-process)}. Under these conditions the reaction path runs far from the valley of stability, out toward the neutron drip line, where nuclei are so neutron-rich that adding one more neutron barely binds at all [ 8 ] . Capture continues, isotope after isotope, until it reaches a nucleus at one of the neutron shell closures — the magic neutron numbers 50, 82 and 126 — where the next capture is…

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