This is the final year of the three year grant cycle The Caltech program has vigorous theory groups (Tasks A, B) These groups receive major support from Caltech - HEP phenomenology and string theory – Gukov, Kapustin, Ooguri, Preskill, Schwarz, Wise
- Particle astrophysics – Carroll, Hirata, Kamionkowski
Our major experimental activities (Tasks C, D, E) are - Electrons: ILC GDE, BABAR, SuperB – Barish, Hitlin, Porter
- Protons: MINOS, Noa, CMS – Newman, Spiropulu
- Non-accelerator: CDMS & SuperCDMS - Golwala
Our main concerns for FY09 are - Ramping up support for Maria Spiropulu and the CMS effort
- Creation of an advanced crystal development laboratory
- Inflation adjustment
Our computing model is predicated on an adiabatic replacement cycle - Non-CMS computing remains important for the BABAR Intense Analysis phase and for MINOS and SuperB
- By replacing a fraction of farm CPU’s each year, we have avoided the need for massive reworking of the system
- To stave off obsolescence, this approach requires us to replace ~1/4 to 1/3 of computing capacity and storage each year
- In FY08 computing equipment funding fell far off this curve
- In FY09 we fell further off the curve
The Caltech program remains strong, with a good mix of experimental opportunities and a powerful theory group The Caltech program remains strong, with a good mix of experimental opportunities and a powerful theory group We continue to play leadership roles in present and future experiments In accord with the P5 report, we are looking in new directions - Particle astrophysics – SuperCDMS (Golwala)
- Next generation neutrino physics – Noa (Newman)
- Next generation flavor physics - SuperB (Hitlin, Porter)
- LHC upgrades (Newman, Spiropulu)
- A future lepton collider
We a actively engaged with the Division Staffing Committee, pointing towards a new junior faculty appointment
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