Research Highlights

Here we provide short descriptive summaries of the major accomplishments and highlights of JINA research so far.

Research Highlights (2015 - 2018)
Research Highlights (2012 - 2014)
Research Highlights (2009 - 2011)
Research Highlights (2006 - 2008)
Research Highlights (2003 - 2005)
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Major Accomplishments 2015 - 2018 MA 1 || MA 2 || Outreach

	Neutrinos Before Collapse		Connecting the Dots: From Nucleosynthesis in Early Massive Stars to the Elemental Abundances of the Most Iron-Poor Stars
	Probing Nuclear Astrophysics with Chemical Evolution		First Beam and Inauguration of CASPAR
	Nuclear experimentalists, theorists, and astrophysicists constrain reaction rates necessary for understanding how massive stars explode		Advanced LIGO and the Origin of the r-Process
	Following the Cosmic Evolution Of Pristine Gas		i-process Nucleosynthesis and Mass Retention Efficiency in He-shell Flash Evolution of Rapidly Accreting White Dwarfs
	First CASPAR Beam on the Horizon		Impact of (α, n) Reactions on Weak r-Process in Neutrino-Driven Winds
	Islands of Non-Explodability and Chemical Evolution		Low-Mass Supernova Triggered the Formation of Our Solar System
	Broken Neutron Link in the Sky		A New Study of One of the First Stars
	Uncertainties in Galactic Chemical Evolution Models		A Rare and Prolific r-Process Event Preserved in an Ancient Dwarf Galaxy
	The Impact of Individual Nuclear Properties on r-process Nucleosynthesis		New Evidence for the i-process in the Early Galaxy
	Predicting charged-particle reaction rates with HABANERO		Tracing the Origins of Stardust in the Nuclear Physics Lab
	Super-AGB stars: A Nuclear Astrophysics Site for the i-Process		Weak-rate Library for Astrophysical Simulations
	The First Age Map of the Galactic Halo		CASPAR Accelerator Assembled Underground
	Hubble Space Telescope Near-Ultraviolet Spectroscopy of Bright CEMP-s Stars		A Speed Trap for Nuclei
	Discovery of the Brightest Ultra-Metal Poor Star		New 3-D model could solve supernova mystery
	Low Energy Fusion Studies for Stellar Carbon Burning		Nuclear Physics Is Needed To Predict White Dwarf Properties

	Improvements for exotic beam experiments at TwinSol		Indirect Studies of (α,p) Reactions along the αp-Process Path and their Influence on Type 1 X-ray Burst Light Curves.
	First Science Result With the JENSA Gas-Jet Target		Radioactive Beam Experiment Sheds Light on Nova Explosions
	Rp-process in X-ray Bursts May Produce Heavier Elements Faster		A Lower Limit on the Heat Capacity of a Neutron Star Core
	Fingerprinting Neutron Stars Through Thermonuclear Bursts		Neutrino Cooling in the Accreted Neutron Star Ocean
	Matter Neutrino Resonance in Neutron Star Merger Remnants		Investigating the Thermal Properties of Nuclear Pasta with Neutron Stars
	Shallow Heating in Neutron Stars		Measurements Alter Our Understanding of Neutron Star Surfaces

	Art 2 Science Camp		Art Beat
	Physics of Atomic Nuclei		Outdoor Artists at St Patrick's Park
	Boy Scout Nuclear Badge Workshop		Partnership with Eastside Connections
	Expanding Your Horizons		Partnership with Madison STEAM Academy
	PAN-CAKE Workshop for Teachers		Portrait Theater Performances
	Science Alive and Countdown Events		JINA-CEE Webinar
	Individualized Art 2 Science		Girl Scout Badge: Get to Know Nuclear
	PAN @ IMSA Intersession 2015		Science Alive, South Bend, IN

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