Nuclear Astrophysics at OSU

Ongoing Research Projects ******

Members of the Nuclear Astrophysics Group

Faculty:

* Richard N. Boyd, boyd@mps.ohio-state.edu

Postdoctoral Researcher:

* Alexander Murphy, asmurphy@mps.ohio-state.edu

Graduate Students:

* Arthur Cole, cole@mps.ohio-state.edu
* Meredith Howard, meredith@pacific.mps.ohio-state.edu
* Edward Smith, edesmith@pacific.mps.ohio-state.edu
* Juergen J. Zach (WEBMASTER), jjzach@campbell.mps.ohio-state.edu

Staff (shared with the other Experimental Nuclear Physics Groups):

* Howard Dyke, Senior Design Engineer, dyke@mps.ohio-state.edu
* Mary Smith, Secretary, msmith@mps.ohio-state.edu

Alumni of the Nuclear Astrophysics Group: former students and staff.

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Papers by the Nuclear Astrophysics Group

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Current research projects of The Nuclear Astrophysics Group

The Observatory for Multi Flavour Neutrinos from Supernovae (OMNIS)

Ongoing Progress:

* Project DAMOCLES - Optimization of OMNIS Detector Maintained by Juergen J. Zach

Group members involved:

* Dr. Richard N. Boyd, Principal Investigator
* Dr. Alexander StJ Murphy, Research Scientist, Experimental Detector Work and OMNIS Webmaster
* Juergen J. Zach, Graduate Student, Monte Carlo Simulations and Detection Schemes for OMNIS

Supernova Early Warning System (SNEWS)

* Dr. Alexander StJ Murphy is the OMNIS Representative to the SNEWS-collaboration

Supernova Tracing in Ice Core Samples

* Arthur Cole is looking for signatures of past supernovae in icecore samples

Interaction of Supernova Neutrinos with Strange Matter in (Proto-) Neutronstars

* Juergen J. Zach is involved in trying to find out what the introduction of strange matter in neutron stars would do to the supernova neutrino signal

Isobaric analogue states

* Dr. Murphy is using levels in a known nucleus (Ti46) to deduce the properties of unknown levels in another nucleus (Cr46). This is so that the V45(p,g)Cr46 reaction rate, which is an important link in the production of Ti46, may be estimated.

Pycnonuclear reactions

* He is also looking into rates in extremely dense, but relatively cold environments (older neutron stars for example)

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Some of the past research projects of The Nuclear Astrophysics Group

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Back to the Nuclear Physics and Astrophysics Experiment Home Page.


Created in 1997 by chloupek@mps.ohio-state.edu

Last modified Aug 2001 by Juergen J. Zach , the GROUP WEBMASTER: jjzach@campbell.mps.ohio-state.edu