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Multidisciplinary Science in the Multimessenger Era
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Astrophysical observations of the cosmos allow us to probe extreme physics and answer foundational questions on our universe. Modern astronomy is increasingly operating under a holistic approach, probing the same question with multiple diagnostics including how sources vary over time, how they appear across the electromagnetic spectrum, and through their other signatures, including gravitational waves, neutrinos, cosmic rays, and dust on Earth. Astrophysical observations are now reaching the point where approximate physics models are insufficient. Key sources of interest are explosive transients, whose understanding requires multidisciplinary studies at the intersection of astrophysics, gravity, nuclear science, plasma physics, fluid dynamics and turbulence, computation, particle physics, atomic, molecular, and optical science, condensed matter and materials science, radiation transport, and high energy density physics. This white paper provides an overview of the major scientific advances that lay at the intersection of physics and astronomy and are best probed through time-domain and multimessenger astrophysics, an exploration of how multidisciplinary science can be fostered, and introductory descriptions of the relevant scientific disciplines and key astrophysical sources of interest.
Forward citations
Cited by 4 Pith papers
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Kilonovae and Long-duration Gamma-ray Bursts
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4th TDAMM Workshop White Paper
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The Heavy Element Enrichment History of the Universe from Neutron Star Mergers with Habitable Worlds Observatory
A whitepaper arguing that HWO, with rapid, deep UV-optical-IR follow-up of gravitational-wave-detected neutron star mergers, could map the cosmic history of r-process enrichment.
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