Opening Speech

• Marcel Demarteau (ANL)

Room: Chicago Ballrooms 8,9,10

Innovation: How It Happens

• Bill Brinkman (DOE Office of Science)

Room: Chicago Ballrooms 8,9,10

Extremes of Electronics

• Kerry Bernstein (IBM, Yorktown Heights)

Room: Chicago Ballrooms 8,9,10

The LHC Detectors: Marvels of Technology

• Sergio Bertolucci (CERN)

Room: Chicago Ballrooms 8,9,10

Probing the Cosmic Frontier with the Cosmic Microwave Background: Current Status and Future Challenges

• John Carlstrom (University of Chicago)

Room: Chicago Ballrooms 8,9,10 Cosmic Microwave Background measurements play a key role in the exploration of the cosmic frontier. The remarkably high degree of isotropy in the CMB led to the inflation theory for the origin of our universe, through exponential expansion of quantum fluctuations at the GUT energy scales. Further CMB measurements showed the curvature of the universe is flat and that the distribution of the primordial scalar fluctuations are nearly, but not exactly, scale invariant, again consistent with inflation. CMB measurements have also provided a full inventory of the components of the energy-density of the universe, showing that dark matter is non-baryonic and confirming that the universe is dominated today by dark energy. The current goal of ongoing and future CMB measurements is to explore the nature of the dark energy and to determine the energy of inflation. The field continues to be driven by advances in detectors and measurement techniques. In particular, the goal of the pola rization measurements to search for the inflationary gravitation waves, is to obtain sensitivities of order tens of nanoKelvins. This talk will review the current status of CMB measurements and the new developments being pursued to probe the inflationary epoch.

Neutrino Physics and Detectors

• Yifang Wang (IHEP)

Room: Chicago 8,9,&10

Direct Dark Matter Physics and Detectors

• Prisca Cushman (University of Minnesota)

Room: Chicago 8,9 &10

Indirect Dark Matter Physics and Detectors

• Jim Buckley (Washington University)

Room: Chicago 8,9,&10

Rare Decay Experiments

• Yoshi Kuno (Osaka University)

Room: Chicago 8,9,&10

Public Lecture: Marvel of Technology: The LHC, machine and experiments

• Lyn Evans (CERN)

Room: Chicago Ballrooms 8/9/10

Detectors for Nuclear Physics

• Susumu Shimoura (University of Tokyo)

Room: Chicago Ballrooms 8,9,10

Double Beta Decay

• Andrea Pocar (University of Massachusetts, Amherst)

Room: Chicago Ballrooms 8,9,10

Gravitational Wave Detection: Past, Present and Future (Astrophysics and Space Instrumentation)

• Sam Waldman (LIGO MIT)

Room: Chicago Ballrooms 8,9,10 The direct detection of gravitaitonal waves (GWs) offers a revolutionary new probe of the most energetic processes in the universe and precision tests of fundamental theories of gravity. Through their detailed waveforms, GWs carry information about their parent neutron stars, supernovae and black holes, opening a window to the unexplored strong-field, strong-curvature regime of general relativity. Several techniques and collaborations are vying to make the first direct detection within the next 5 to 10 years. In this talk, I will describe: 1. the first-generation, kilometer scale LIGO and Virgo interferometers that have demonstrated the sub-attometer displacement sensitivity (< 10^{-18} m/ Hz^{1/2}) and continuous operation (> 75\% duty factor) needed to detect GWs from beyond the Virgo cluster; 2. the Pulsar timing arrays that have demonstrated the sub-microsecond timing residuals and multi-year observations needed to detect a passing GW's effect; and 3. the detection of the of a GW's imprint on the polarization of the cosmic microwave background.

Synchrotron and X-Ray Applications

• Klaus Attenkofer (Argonne National Laboratory)

Room: Chicago Ballrooms 8,9,10

Dinner

• Marcel Demarteau (Fermi National Accelerator Lab. (Fermilab))

Room: Mid America Club

Detectors for Future Colliders

• Hitoshi Yamamoto

Room: Chicago Ballrooms 8,9,10

DAQ and Triggering

• Wesley Smith (University of Wisconsin)

Room: Chicago Ballrooms 8,9,10

Applications outside of HEP

• Patrick LeDu

Room: Chicago Ballrooms 8,9,10

Applications of Analog Circuit Design to Life as a Scientist in the United States Congress

• G. William (Bill) Foster (fmr. Rep. U.S. congress)

Room: Chicago Ballrooms 8,9,10

Closing Speech

• Tiehui Ted Liu (Fermilab)

Room: Chicago Ballrooms 8,9,10

3D Satellite Meeting: Introduction

• Grzegorz Deptuch (FERMILAB)

Room: Sheraton Hotel

3D Satellite Meeting: Flavors of the 3D-IC technology and where it is applicable

• Paul Franzon (NCSU)

Room: Sheraton Hotel

3D Satellite Meeting: 3D technology developments in Europe and European Union supported efforts

• Hans Gunther Moser (MPI)

Room: Sheraton Hotel

3D Satellite Meeting: 3D landscape in Japan

• Masahiro Aoyagi (AIST (Japan))

Room: Sheraton Hotel

3D Satellite Meeting: TSV revolution and Fermilab’s MPW experience

• Ray Yarema (FNAL)

Room: Sheraton Hotel

3D Satellite Meeting: Testimonial Talks

• INFN, IN2P3, DoE

Room: Sheraton Hotel

3D Satellite Meeting: Q&A, Panel Discussion and Coffee Room: Sheraton Hotel

3D Satellite Meeting: SOI technology for monolithic and 3D integrated detectors

• Yasuo Arai (KEK)

Room: Sheraton Hotel

3D Satellite Meeting: 3D-IC enabler of advanced focal planes

• Chenson Chen (MIT-LL (USA))

Room: Sheraton Hotel

3D Satellite Meeting: 3D-IC for real chips and prospectives

• Bob Patti (Tezzaron)

Room: Sheraton Hotel

3D Satellite Meeting: The Monolithic 3D-IC

• Zvi Or-Bach (MonolithIC 3D)

Room: Sheraton Hotel

3D Satellite Meeting: Q&A, Panel Discussion and Tea Room: Sheraton Hotel

3D Satellite Meeting: Conclusions Room: Sheraton Hotel