The quantum spectral method: from atomic orbitals to classical self-force

Majed Khalaf, Ofri Telem*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

Can classical systems be described analytically at all orders in their interaction strength? For periodic and approximately periodic systems, the answer is yes, as we show in this work. Our analytical approach, which we call the Quantum Spectral Method, is based on a novel application of Bohr’s correspondence principle, obtaining non-perturbative classical dynamics as the classical limit of quantum matrix elements. A major application of our method is the calculation of self-force as the classical limit of atomic radiative transitions. We demonstrate this by calculating an adiabatic electromagnetic inspiral, along with its associated radiation, at all orders in the multipole expansion. Finally, we propose a future application of the Quantum Spectral Method to compute scalar and gravitational self-force in Schwarzschild, analytically.

Original languageEnglish
Article number53
JournalJournal of High Energy Physics
Volume2024
Issue number9
DOIs
StatePublished - Sep 2024

Bibliographical note

Publisher Copyright:
© The Author(s) 2024.

Keywords

  • Black Holes
  • Classical Theories of Gravity

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