The Second TAMA Workshop on Gravitational Wave Detection

First Circular

October 19 (Tue) to 22 (Fri) in 1999

National Olympics Memorial Youth Center, Tokyo, Japan

International workshop on experiments and developments for gravitational wave detection

Objective
Detecting gravitational waves has been a dream for a long time in the field of physics and astronomy, and recent developments make us very confident of it becoming a reality. In particular, we have reached the stage where we can set out a concrete plan for a large-scale interferometer which should be able to detect gravitational waves from plausibly expected sources. We wish to establish the field of "gravitational wave astronomy" which will afford new knowledge of the Universe that cannot be obtained from other more traditional techniques such as optical and radio astronomy.
Several projects have already started throughout the world for the construction of large- scale laser interferometric gravitational wave detectors such as those of LIGO, VIRGO, and GEO. We in Japan started the project , called the TAMA project, to develop a laser interferometer with a baseline of 300m (TAMA300) in 1994; this year, 1999 is the final year of this five-year project.
The workshop will be organized similar to the first TAMA Workshop in 1996. The emphasis of the workshop this time is on discussion of the results of TAMA300 (TAMA300 is expected to be in the final phase of completion at the time of the workshop), as well as on the current status of other projects. In addition, there will be discussions of both developed and developing advanced techniques in the various fields necessary for improving the sensitivity of gravitational wave detectors. The workshop will have twelve invited speakers and some contributed papers, and no poster session.

Organization
Chair person: Prof. Yoshihide Kozai, the leader of the TAMA project

International Advisory Committee:
B. Allen                UWM
B. Barish               Caltech 
D. Blair                UWA
S. Bonazzola            Observatoire Paris-Meudon
V. Braginskii           Moscow
A. Brillet              CNRS-Nice
R. Byer                 Stanford
M. Cerdonio             Padova
K. Danzmann             Hannover
S. Finn                 Penn State
A. Giazotto             INFN Pisa
W. Hamilton             LSU
J. Hough                Glasgow
J. Sandeman             ANU
G. Sanders              Caltech
B. Schutz               Potsdam
K. Thorne               Caltech
G. Veneziano            CERN
R. Weiss                MIT

Program/Organizing Committee:
M. Fujimoto             NAOJ
N. Kanda                MUE
S. Kawamura(Chair)      NAOJ
N. Kawashima            Kinki Univ.
Y. Kozai                NAOJ
K. Kuroda               ICRR
S. Meshkov              Caltech
N. Mio(Co-chair)        Univ. Tokyo
T. Nakamura             YITP
M. Ohashi               ICRR
R. Takahashi            NAO
K. Tsubono              Univ. Tokyo
K. Ueda                 ILS

Conference Site
The National Olympics Memorial Youth Center (NYC) in the city of Tokyo has been chosen as the conference venue; this center is a national youth educational facility established with the aims of promoting the sound development of youth and youth education in Japan and has an international conference hall and accommodations. Detailed information can be obtained from the Web page of the center; its URL is http://www.nyc.go.jp/eng/e00101.html.

Program
Topics that will be presented and discussed are as follows: project status, laser and optics, interferometer, isolation and thermal noise, theory and data analysis, others. Twelve invited talks and contributed talks are planned. The TAMA Session is planned for the second day of the workshop; the session will be held at the campus of National Astronomical Observatory of Japan (NAOJ) in Mitaka where the TAMA 300 detector is being developed and the TAMA Site Tour is also scheduled.

The following is a tentative outline of the program.

Tuesday, Oct 19 
        Morning: opening talks, project status
        Afternoon: laser and optics.

Wednesday, Oct 20
        TAMA Session at NAOJ

Thursday, Oct 21
        Morning: interferometer
        Afternoon: isolation and thermal noise (banquet)

Friday, Oct 22
        Morning: data analysis
        Afternoon: other topics, closing talks.

List of Invited Speakers:
P. Bender               JILA
J. Camp                 Caltech 
V. Cook                 NSF
F. Frasconi             INFN Pisa
P. Fritschel            MIT
A. Heidmann             Paris
S. Rowan                Stanford
B. Sathyaprakash        Cardiff University
S. Scott                ANU
K. Strain               Glasgow 
B. Willke               Hannover
J. Winterflood          UWA

Attendance and Registration
Participants are required to submit a registration form to the conference office before Jun 30th, 1999; the participants who wish to contribute are also requested to submit the title, the author(s) and the abstract within 200 words. The submission via e-mail is strongly recommended. The registration fee is 20,000 yen ( including the fee for banquet and proceedings). The corresponding address for the registration is as follows:

Secretariat of the 2nd TAMA Workshop
National Astronomical Observatory of Japan
Mitaka, Tokyo, 181-8588, JAPAN
E-mail: tamaws@gravity.mtk.nao.ac.jp
Phone: +81-422-34-3620
Fax: +81-422-34-3793

Accommodation
Since accommodation is limited, participants who want to stay in the conference venue should specify the dates when they will stay, in the registration form. Since, as mentioned above, NYC is established for the education of young people, the accommodations for men and women are separated. If this situation is inconvenient, there are many hotels in the city of Tokyo that are not far from NYC.

Further Information
Please contact the conference secretariat:

Secretariat of the 2nd TAMA Workshop
National Astronomical Observatory of Japan
Mitaka, Tokyo, 181-8588, JAPAN
E-mail: tamaws@gravity.mtk.nao.ac.jp
Phone: +81-422-34-3620
Fax: +81-422-34-3793
WWW: http://tamago.mtk.nao.ac.jp/tama/tamaws/tamaws2.html