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Dr. Michael Strickland's group will participate in a new Topical Theory Collaboration funded by DOE’s Office of Nuclear Physics to explore the behavior of heavy flavor particles. The collaboration will receive $2.5 Million from the DOE Office of Science, Office of Nuclear Physics, over five years. That funding will provide partial support for six graduate students and three postdoctoral fellows at 10 institutions, as well as a senior staff position at one of the national laboratories. It will also establish a bridge junior faculty position at �鶹��Ƶ.

Neutron stars are some of the densest objects in the universe, and as such, the conditions at the cores of these extreme objects are impossible to reproduce on Earth. However, we can use data from the Laser Interferometer Gravitational Wave Observatory (LIGO) and the Virgo gravitational wave detector to gain insights into the physics of neutron stars.

Up until approximately 10^(-5) seconds after the Big Bang, the Universe was is a primordial state of matter called a quark-gluon plasma (QGP).  This is due to the fact that the early Universe was extremely hot and in such a hot environment normal matter, e.g., atoms, atomic nuclei, and even neutrons and protons, did not exist.

The National Institutes of Health (NIH) recently awarded a $1.86 million grant to Thorsten-Lars Schmidt, Ph.D., to develop molecular tools that help researchers to understand membrane proteins.  As an add-on the NIH awarded Dr. Schmidt an instrumentation grant for a high-end Atomic Force Microscope.

The National Institutes of Health (NIH) recently awarded a $1.86 million grant to Thorsten-Lars Schmidt, Ph.D., to develop molecular tools that help researchers to understand membrane proteins.  As an add-on the NIH awarded Dr. Schmidt an instrumentation grant for a high-end Atomic Force Microscope.

The National Institutes of Health recently awarded a $1.86 million grant to Thorsten-Lars Schmidt to develop molecular tools that help researchers to understand membrane proteins. This is the first time a professor at �鶹��Ƶ has been awarded an R35, which provides promising researchers with a five-year funding for a broader research program, rather than funding a specific project. This gives investigators a lot of freedom to develop new research directions as opportunities arise, rather than being bound to specific aims of a more narrow study.

Edwin Duckworth, a physics doctoral student in the College of Arts and Sciences at �鶹��Ƶ, is among 65 students from 29 states recently selected for funding by the Department of Energy’s (DOE) Office of Science Graduate Student Research (SCGSR) program. The program aspires to “address societal challenges at national and international scale.”

What happens when two neutron stars collide? What extreme densities and temperatures are reached? What new states of matter exist within the core of a neutron star? One �鶹��Ƶ College of Arts and Sciences theoretical astrophysicist, Veronica Dexheimer, associate professor in the Department of Physics, is diving headfirst into these questions as a co-principal investigator collaborating with her peers at multiple institutions on a recently funded cyberinfrastucture research grant project.