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19 August 2002 LSC Meeting — LIGO Hanford Obse rvatory 1 Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO Group Group Petition to Join the LIGO Science Collaboration Steven Penn Hobart and William Smith Colleges LIGO-G020391-00-Z

Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

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Page 1: Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

19 August 2002 LSC Meeting — LIGO Hanford Observatory 1

Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO GroupGroup

Petition to Join the LIGO Science Collaboration

Steven PennHobart and William Smith Colleges

LIGO-G020391-00-Z

Page 2: Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

19 August 2002 LSC Meeting — LIGO Hanford Observatory 2

Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO GroupGroup

• Hobart, founded 1820, and William Smith, founded 1908, are nominally independent, unisex schools, which have been merged as a single coeducational college for 60 years.

• 2,500 students. Strong focus on liberal arts, chemistry, and enviro. science.

• Located in Geneva, NY on Seneca Lake, largest of the Finger Lakes, and ancestral home of the Seneca Nation.

• Influence of nearby Seneca Falls. Elizabeth Blackwell, the first woman in US to receive an MD, graduated from Geneva College.

• President’s house was a major stop on the Underground Railroad.

Basics of HWS:

Page 3: Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

19 August 2002 LSC Meeting — LIGO Hanford Observatory 3

Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO GroupGroup

Recent Events at HWS

New President Mark Gearan, head of Peace Corp during Clinton, has initiated a major campaign to reinvigorate the colleges.

• New Chemistry building

• New Library Wing

• New Sociology/Psychology building• $100 million raised to improve research and education facilities• New “Finger Lakes Institute” planned• New Physics building, larger dept. planned

Page 4: Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

19 August 2002 LSC Meeting — LIGO Hanford Observatory 4

Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO GroupGroup

Physics at HWS

• Small department: 5 faculty, 15 majors. Don Spector (Harvard, particle theorist), Ted Allen (Caltech, particle/string theorist), Larry Campbell (Carnegie Mellon, nuclear/optics), Michael Faux (Penn, string theorist), and Steven Penn (MIT, nuclear/LIGO).

• Administration, campaign to strengthen sciences, plans to increase faculty to 6 (2 new experimenters), and new building.

• Physics, Chemistry, Biology, and Env. Science jointly apply for new NSF grant to increase majors.

Page 5: Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

19 August 2002 LSC Meeting — LIGO Hanford Observatory 5

Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO GroupGroup

Support for LIGO group at HWS

• Start-up of $100k and renovated lab space.• Agreement to match all grants. No ceiling.• No overhead.• Full-time technician.• Arrange classes to allow 1/2 time at SU.• Encourage (partial support?) for a post-doc.

Page 6: Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

19 August 2002 LSC Meeting — LIGO Hanford Observatory 6

Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO GroupGroup

Thermal Noise Research

• Coating Loss: (Glasgow, MIT, Stanford, Syracuse)– Shown that coating loss due to bulk loss, mostly tantala– Future tests:

• Other materials (Niobia/Silica, Alumina/Silica, …)• Varied Methods: Doping tantala, optimized annealing

• Silica Surface Loss and Annealing– Q vs. V/S has reached Q = 84 million for V/S > 2 mm– Future tests:

• Annealing• other FS varieties, esp. Supersil SV super-low OH

• Investigate thermal noise issues in Sapphire

• Continued collaboration with SU group

Page 7: Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

19 August 2002 LSC Meeting — LIGO Hanford Observatory 7

Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO GroupGroup

Detector Characterization Research

Bilinear Coupling Investigation

• BicoMon: a data monitor which calculates the bicoherence & bispectrum. Used to detect bilinear processes, quadratic phase coupling, frequency/phase noise.

• Future directions: to expand BicoMon into a more complete of suite of second-order statistics tool, including gaussianity & linearity tests and bicepstrum.

Page 8: Hobart & William Smith Colleges LIGO Group 19 August 2002LSC Meeting — LIGO Hanford Observatory1 Petition to Join the LIGO Science Collaboration Steven

19 August 2002 LSC Meeting — LIGO Hanford Observatory 8

Hobart & William Smith Colleges LIGO Hobart & William Smith Colleges LIGO GroupGroup

Summary

• Continued program of LIGO research on coating loss, thermal noise for Advanced LIGO, and detector characterization.

• HWS is being very supportive in funds and facilities.

• HWS location allows continuation of valuable collaborative work with Syracuse.