%AChidester, Morgan%AFarag, Ebraheem%ATimmes, F.%BJournal Name: The Astrophysical Journal; Journal Volume: 935; Journal Issue: 1 %D2022%I %JJournal Name: The Astrophysical Journal; Journal Volume: 935; Journal Issue: 1 %K %MOSTI ID: 10358252 %PMedium: X %TOn Trapped Modes in Variable White Dwarfs as Probes of the 12 C(α, γ) 16 O Reaction Rate %XAbstract We seek signatures of the current experimental 12 C α , γ 16 O reaction rate probability distribution function in the pulsation periods of carbon–oxygen white dwarf (WD) models. We find that adiabatic g-modes trapped by the interior carbon-rich layer offer potentially useful signatures of this reaction rate probability distribution function. Probing the carbon-rich region is relevant because it forms during the evolution of low-mass stars under radiative helium-burning conditions, mitigating the impact of convective mixing processes. We make direct quantitative connections between the pulsation periods of the identified trapped g-modes in variable WD models and the current experimental 12 C α , γ 16 O reaction rate probability distribution function. We find an average spread in relative period shifts of Δ P / P ≃ ±2% for the identified trapped g-modes over the ±3 σ uncertainty in the 12 C α , γ 16 O reaction rate probability distribution function—across the effective temperature range of observed DAV and DBV WDs and for different WD masses, helium shell masses, and hydrogen shell masses. The g-mode pulsation periods of observed WDs are typically given to six to seven significant figures of precision. This suggests that an astrophysical constraint on the 12 C α , γ 16 O reaction rate could, in principle, be extractable from the period spectrum of observed variable WDs. %0Journal Article