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arXiv · 1811.06157

Perspectives on Astrophysics Based on Atomic, Molecular, and Optical (AMO) Techniques

Abstract

About two generations ago, a large part of AMO science was dominated by experimental high energy collision studies and perturbative theoretical methods. Since then, AMO science has undergone a transition and is now dominated by quantum, ultracold, and ultrafast studies. But in the process, the field has passed over the complexity that lies between these two extremes. Most of the Universe resides in this intermediate region. We put forward that the next frontier for AMO science is to explore the AMO complexity that describes most of the Cosmos.

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Daniel Wolf Savin, James F. Babb, Paul M. Bellan, Crystal Brogan, Jan Cami, Paola Caselli, Lia Corrales, Gerardo Dominguez, Steven R. Federman, Chris J. Fontes, Richard Freedman, Brad Gibson, Leon Golub, Thomas W. Gorczyca, Michael Hahn, Sarah M. Hörst, Reggie L. Hudson, Jeffrey Kuhn, James E. Lawler, Maurice A. Leutenegger, Joan P. Marler, Michael C. McCarthy, Brett A. McGuire, Stefanie N. Milam, Nicholas A. Murphy, Gillian Nave, Aimee A. Norton, Anthony Papol, John C. Raymond, Farid Salama, Ella M. Sciamma-O'Brien, Randall Smith, Chad Sosolik, Clara Sousa-Silva, Phillip C. Stancil, Frank Timmes, Virginia L. Trimble, Bradford J. Wargelin. 2018-11-15. Perspectives on Astrophysics Based on Atomic, Molecular, and Optical (AMO) Techniques. https://arxiv.org/abs/1811.06157

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