N3AS Research Themes

Neutrino Physics (PFC Major Activity 1)

Thumbnail for Neutrino Physics. Credit: Australian Astronomical Observatory


Beyond-the-standard model (BSM) physics of neutrinos, including their mixing phenomena on earth and in extreme astrophysical environments; the absolute mass scale and the eigenstate behavior under particle-antiparticle conjugation, and the implication of mass and lepton number violation for cosmological evolution; and the relevance of neutrinos to astrophysics both in transporting energy and lepton number, and as a probe of the otherwise hidden physics that governs the cores of stars and compact objects.

Nucleosynthesis (PFC Major Activity 2)

Figure thumbnail showing exponential reach.

The synthesis of light nuclei in the Big Bang constrains cosmological parameters such as the baryon-to-photon ratio and new, beyond-the-standard-model physics, such as sterile neutrinos. The synthesis of heavy nuclei depends both on our understanding of highly explosive, transient astrophysical environments and the properties of exotic nuclei that will soon be probed at FRIB. A quantitative theory of such nucleosynthesis will constrain the history of star formation, supernovae, mergers, and other events that eject newly synthesized elements into the interstellar medium.


Dense Matter and Neutron Stars (PFC Major Activity 3)

Thumbnail for Dense Matter and Neutron Stars. Credit: NASA and STSci

The announcement on 17 August 2017 by LIGO and Virgo of the detection of gravitational waves from a binary neutron star merger, followed by the observation of electromagnetic signals from the associated kilonova as well as a short-duration gamma-ray burst, ushered in a new era of multi-messenger astrophysics and cosmology. In combination with observations of cold neutron stars of nearly two solar masses by Shapiro delay, and of “black-widow” systems hinting of even higher masses, the observations are placing important new constraints on the equation of state of nuclear matter. Current and anticipated observations provide unprecedented opportunities to probe nuclear matter at densities and isospins not otherwise reachable, and to relate its properties to those we measure in laboratory nuclei.

Dark Matter (PFC Major Activity 4)

 Definitive evidence that dark matter (DM) dominates our universe is the second demonstration of BSM physics. Nuclear physics can play an important role in this field by helping direct-detection experimenters understand the variety and nature of the possible responses of their nuclear targets, by connecting the stellar processes we study to the feedback mechanisms that can alter galactic structure, and by contributing to the understanding of composite dark matter in cases where lattice QCD methods are relevant.

Astrophysical Simulations (PFC Major Activity 5)

Thumbnail for Astrophysical Simulations. Credit: National Science Foundation/LIGO/Sonoma State University/A. Simonnet.

The connections N3AS investigators strive to make between observations and fundamental neutrino, dense matter, and dark matter physics require high-fidelity simulations of supernovae, mergers, kilonovae, cooling neutrino stars, and the Big Bang. An important goal of N3AS is to further develop such simulation tools, incorporating into these models the most advanced treatments of the underlying neutrino and nuclear matter microphysics.