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Recorded as part of the White Dwarfs from Physics to Astrophysics (#whitedwarfs-c22) conference at KITP on November 14 - 17, 2022 in Santa Barbara, CA. Astrometric, photometric and spectroscopic all-sky surveys provide the first complete, unbiased view of the Galactic population of the most abundant type of stellar remnants: white dwarfs. This wealth of observational data provides an array of opportunities to use white dwarfs as probes of a wide range of astrophysics, including the formation and evolution of stars and planets, the star formation rate of the Galaxy, and the populations of low-frequency gravitational wave sources and progenitors of thermonuclear supernovae. These applications require improved models of these electron-degenerate stars, which in turn rely on developments in the relevant input physics, including equations of state and opacities. This conference will provide a joint platform for experts in the observational and theoretical study of white dwarfs, scientists working on the underlying fundamental physics, and astronomers using white dwarfs as diagnostic tools to gain a panoramic overview of the state-of-the-art, to identify remaining limitations of the current models, and to explore novel scientific opportunities arising from the new data. Coordinators: Ken Shen and Alejandra Romero More information: https://www.kitp.ucsb.edu/activities/whitedwarfs-c22 __________________________________ Learn more at: https://www.kitp.ucsb.edu Follow @KITP_UCSB for updates on Twitter: https://twitter.com/kitp_ucsb __________________________________ The position of the KITP is that ownership and copyright of all online material -- slides, text, audio, video, and podcasts -- belongs to the author. KITP is providing dissemination for these materials but does not claim ownership. Any person citing these materials for scholarly purposes should provide an appropriate scholarly reference.

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