Perspectives on Astrophysics Based on Atomic, Molecular, and Optical (AMO) Techniques. (arXiv:1811.06157v1 [physics.atom-ph])
<a href="http://arxiv.org/find/physics/1/au:+Savin_D/0/1/0/all/0/1">Daniel Wolf Savin</a>, <a href="http://arxiv.org/find/physics/1/au:+Babb_J/0/1/0/all/0/1">James F. Babb</a>, <a href="http://arxiv.org/find/physics/1/au:+Bellan_P/0/1/0/all/0/1">Paul M. Bellan</a>, <a href="http://arxiv.org/find/physics/1/au:+Brogan_C/0/1/0/all/0/1">Crystal Brogan</a>, <a href="http://arxiv.org/find/physics/1/au:+Cami_J/0/1/0/all/0/1">Jan Cami</a>, <a href="http://arxiv.org/find/physics/1/au:+Caselli_P/0/1/0/all/0/1">Paola Caselli</a>, <a href="http://arxiv.org/find/physics/1/au:+Corrales_L/0/1/0/all/0/1">Lia Corrales</a>, <a href="http://arxiv.org/find/physics/1/au:+Dominguez_G/0/1/0/all/0/1">Gerardo Dominguez</a>, <a href="http://arxiv.org/find/physics/1/au:+Federman_S/0/1/0/all/0/1">Steven R. Federman</a>, <a href="http://arxiv.org/find/physics/1/au:+Fontes_C/0/1/0/all/0/1">Chris J. Fontes</a>, <a href="http://arxiv.org/find/physics/1/au:+Freedman_R/0/1/0/all/0/1">Richard Freedman</a>, <a href="http://arxiv.org/find/physics/1/au:+Gibson_B/0/1/0/all/0/1">Brad Gibson</a>, <a href="http://arxiv.org/find/physics/1/au:+Golub_L/0/1/0/all/0/1">Leon Golub</a>, <a href="http://arxiv.org/find/physics/1/au:+Gorczyca_T/0/1/0/all/0/1">Thomas W. Gorczyca</a>, <a href="http://arxiv.org/find/physics/1/au:+Hahn_M/0/1/0/all/0/1">Michael Hahn</a>, <a href="http://arxiv.org/find/physics/1/au:+Horst_S/0/1/0/all/0/1">Sarah M. H&#xf6;rst</a>, <a href="http://arxiv.org/find/physics/1/au:+Hudson_R/0/1/0/all/0/1">Reggie L. Hudson</a>, <a href="http://arxiv.org/find/physics/1/au:+Kuhn_J/0/1/0/all/0/1">Jeffrey Kuhn</a>, <a href="http://arxiv.org/find/physics/1/au:+Lawler_J/0/1/0/all/0/1">James E. Lawler</a>, <a href="http://arxiv.org/find/physics/1/au:+Leutenegger_M/0/1/0/all/0/1">Maurice A. Leutenegger</a>, <a href="http://arxiv.org/find/physics/1/au:+Marler_J/0/1/0/all/0/1">Joan P. Marler</a>, <a href="http://arxiv.org/find/physics/1/au:+McCarthy_M/0/1/0/all/0/1">Michael C. McCarthy</a>, <a href="http://arxiv.org/find/physics/1/au:+McGuire_B/0/1/0/all/0/1">Brett A. McGuire</a>, <a href="http://arxiv.org/find/physics/1/au:+Milam_S/0/1/0/all/0/1">Stefanie N. Milam</a>, <a href="http://arxiv.org/find/physics/1/au:+Murphy_N/0/1/0/all/0/1">Nicholas A. Murphy</a>, <a href="http://arxiv.org/find/physics/1/au:+Nave_G/0/1/0/all/0/1">Gillian Nave</a>, <a href="http://arxiv.org/find/physics/1/au:+Norton_A/0/1/0/all/0/1">Aimee A. Norton</a>, <a href="http://arxiv.org/find/physics/1/au:+Papol_A/0/1/0/all/0/1">Anthony Papol</a>, <a href="http://arxiv.org/find/physics/1/au:+Raymond_J/0/1/0/all/0/1">John C. Raymond</a>, <a href="http://arxiv.org/find/physics/1/au:+Salama_F/0/1/0/all/0/1">Farid Salama</a>, <a href="http://arxiv.org/find/physics/1/au:+Sciamma_OBrien_E/0/1/0/all/0/1">Ella M. Sciamma-O&#x27;Brien</a>, <a href="http://arxiv.org/find/physics/1/au:+Smith_R/0/1/0/all/0/1">Randall Smith</a>, <a href="http://arxiv.org/find/physics/1/au:+Sosolik_C/0/1/0/all/0/1">Chad Sosolik</a>, <a href="http://arxiv.org/find/physics/1/au:+Sousa_Silva_C/0/1/0/all/0/1">Clara Sousa-Silva</a>, <a href="http://arxiv.org/find/physics/1/au:+Stancil_P/0/1/0/all/0/1">Phillip C. Stancil</a>, <a href="http://arxiv.org/find/physics/1/au:+Timmes_F/0/1/0/all/0/1">Frank Timmes</a>, <a href="http://arxiv.org/find/physics/1/au:+Trimble_V/0/1/0/all/0/1">Virginia L. Trimble</a>, <a href="http://arxiv.org/find/physics/1/au:+Wargelin_B/0/1/0/all/0/1">Bradford J. Wargelin</a>

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.

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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