N3AS – Network for Neutrinos, Nuclear Astrophysics, and Symmetries

Collaboration
N3AS is training a new generation of postdoctoral fellows in key interdisciplinary areas important to astrophysics and cosmology.

Research
Learn about our researchers' focus on neutrino physics, nucleosynthesis, dense matter, dark matter, and more.

Browse Publications
Search and view a database of N3AS collaborators' research.

Popular Science Articles
Start discovering these topics with accessible online articles.

The Network for Neutrinos, Nuclear Astrophysics, and Symmetries (N3AS) is a multi-institutional collaboration dedicated to recruiting and training postdoctoral researchers interested in neutrino physics and astrophysics, nuclear astrophysics topics ranging from supernova and neutron star modeling to dark matter, and fundamental symmetries. The collaboration is funded by the National Science Foundation and the Heising-Simons Foundation.

Our network fosters diversity, equity, and inclusion. We welcome scientists of all identities and are committed to creating an inclusive environment for individuals of underrepresented backgrounds.

May

Implicit correlations within phenomenological parametric models of the neutron star equation of state

Speaker(s): Isaac Legred (Caltech)

| 12:00 pm

Pacific

May

The r‐process and the nuclear EOS after aLIGO’s third observing run

Organizer(s): D. Radice, J. Read, L. Roberts

Location: Institute of Nuclear Theory (INT), University of Washington

| 9:00 am

Pacific

Now Accepting Applications: 2022 N3AS Summer School
The N3AS-sponsored Summer School on Multi-Messenger Astrophysics is intended for graduate students and beginning postdoctoral researchers from theory, experiment, or observation.
Entanglement and correlations in fast collective neutrino flavor oscillations
Collective neutrino oscillations play a crucial role in transporting lepton flavor in astrophysical settings like supernovae and neutron star binary merger remnants, which are characterized by large neutrino densities. In […]
Large and massive neutron stars: Implications for the sound speed in dense QCD
How big are neutron stars? Precise measurements of the size of neutron stars are required for having a solid grasp on the state of the densest material in their interiors, and for differentiating between theoretical models.

Network for Neutrinos, Nuclear Astrophysics, and Symmetries (N3AS)

Collaboration

Research

Browse Publications

Popular Science Articles

About N3AS

Upcoming Events

Implicit correlations within phenomenological parametric models of the neutron star equation of state

The r‐process and the nuclear EOS after aLIGO’s third observing run

N3AS Newscenter

Now Accepting Applications: 2022 N3AS Summer School

Entanglement and correlations in fast collective neutrino flavor oscillations

Large and massive neutron stars: Implications for the sound speed in dense QCD

Collaboration

Research

Resources

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