Current CCAPP research interests include large scale structure, GRBs, AGN, the IGM,
gravitational lenses, dark energy and dark matter, ultra-high energy cosmic rays and
gamma-rays, formation and evolution of elements, and neutrino astrophysics/cosmology.
On a quarterly basis, CCAPP will accept applications soliciting funding for CCAPP science initiatives.
The proposals can be to support ongoing research or for R&D in support of future research and
should include a description of the work and required support.
See CCAPP Funding Proposals to apply.
In addition to well-equipped laboratories for detector development and construction, facilities at OSU include membership in the AUGER, ANITA, and GLAST collaborations, a 1/6 observing share of the Large Binocular Telescope, a 1/4 share of MDM observatory, membership in the SMARTS consortium, a 48-node Beowulf cluster, and access to the Ohio Supercomputing Center.
CCAPP-Dark Energy Strategy
- In its first year of operation, members of CCAPP will design a Dark Energy Strategy, possibly joining proposed experiments like the Dark Energy Survey and/or Large Synoptic Survey Telescope, optimally leveraging OSU's pre-existing investments in the Sloan Digital Sky Survey, the Large Binocular Telescope, and expertise from our high energy experimental and observational and theoretical cosmology groups. Through CCAPP, OSU will play a major role in dark energy science addressing the question ``What is the Dark Energy?'', positioning itself to be a leader in the next generation of Dark Energy Experiments.
- In addition to initiating a dark energy program, CCAPP will initiate a focused, vigorous visitor program coupled with small workshops (run cooperatively with OCTS) whose goal is to identify additional projects where OSU’s unique Astronomy and Physics connections can make a significant impact. With an eye towards maximizing return from our current investments (e.g., in the LBT, ISL, and the ANITA, AUGER, and GLAST experiments), potential areas for investigation include:
- The Nature of Dark Matter, as probed by large scale structure, gravitational lensing, deep underground science, and high energy colliders
- The Birth and Growth of the Universe, as imaged by the cosmic microwave background, optical and infrared observations of the first galaxies and quasars, and as reflected in chemical evolution.
- The Coming (of) Age of Ultra-High Energy Astronomy: Black Holes, the Creation of the Highest Energy Particles, and Extreme Astrophysical Environments