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Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet, J. Tiedje http://www. dusel .org

Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

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Page 1: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Deep Underground Science and Engineering Lab

Hamish Robertson for the DUSEL S1 P/Is:

E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B.

Sadoulet, J. Tiedje http://www.dusel.org

Page 2: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

The NSF solicitations 2004-6

Four NSF directorates – MPS, GEO, ENG, BIO

S1 – Research definition and associated infrastructure requirements.

S2 – Site development and conceptual design.

8 proposals “down-selected” to 2 sites, $500 k each.

S3 – Site specific, detailed infrastructure plan for science and engineering for a single site.

Earliest MRE funding available – beginning FY 2009

~ a few X 108 $ for lab plus experiments.

Page 3: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

PhysicsGeosciences &

Engineering

Geomicrobiology

Three Major Research Areas

Page 4: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Physics: the Big Questions

• What is the dark matter? • What is the nature of the dark energy? • How did the universe begin? • Did Einstein have the last word on gravity? • What are the masses of the neutrinos, and how have they

shaped the evolution of the universe? • How do cosmic accelerators work and what are they

accelerating? • Are protons unstable? • Are there new states of matter at exceedingly high density

and temperature? • Are there additional spacetime dimensions? • How were the elements from iron to uranium made?• Is a new theory of matter and light needed at the highest

energies?

Page 5: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Physics: the Big Questions

• What is the dark matter? • What is the nature of the dark energy? • How did the universe begin? • Did Einstein have the last word on gravity? • What are the masses of the neutrinos, and how have they

shaped the evolution of the universe? • How do cosmic accelerators work and what are they

accelerating? • Are protons unstable? • Are there new states of matter at exceedingly high density

and temperature? • Are there additional spacetime dimensions? • How were the elements from iron to uranium made?• Is a new theory of matter and light needed at the highest

energies?

Page 6: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Hime & Mei astro-ph/0512125

Physicists want:•Cosmic-ray Shielding•Seismic quiet•Low radioactivity•Access

Data: Hime & Mei, astro-ph/0512125Curve: Miyake, N.Cim. 32, 1505 (1964)

Page 7: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,
Page 8: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Scientific

Findings

Page 9: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Progra-matic

Findings

Page 10: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Recommendation I

Page 11: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Recommendation II

Page 12: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Recommendation III

Page 13: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Volumes of Lab Space

Page 14: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

DUSEL S2 proposed sites

Cascades

SNOLAB

Kimballton

Soudan

San Jacinto

WIPP

Homestake

Henderson

Page 15: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

DUSEL S3 competitors

Cascades

SNOLAB

Kimballton

Soudan

San Jacinto

WIPP

Homestake

Henderson

Page 16: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Major Opportunity for Neutrino Physics

• Double beta decay, solar neutrinos, other neutrino research need – Support– Institutional Home

• R&D support coming soon (NSF ~$4M, DOE NP ~$1M, DOE HEP ~$5M)

• MREFC concept includes ~$250M (!) for new experiments.

Page 17: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Physics Program • Dark matter • Neutrinoless Double Beta Decay:

– Lepton number violation, matter-antimatter transition in early universe

– Mass of the neutrino• Low-energy neutrinos

– Solar neutrino spectrum, CNO– Sterile neutrinos– Luminosity of future sun– Geoneutrinos– Supernova neutrinos

• Low-cross-section accelerator facility (in addition to LUNA)

• Low background counting– Physics– National security

• CP Violation, Hierarchy, Nucleon Decay: Mega-detector

Page 18: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

S1 Working Groups – PhysicsDetermine the scientific reach of DUSEL

Dark Matter Dan Akerib

(Case Western Reserve U.) Elena Aprile (Columbia U.)

Low-Energy Neutrinos Tom Bowles (LANL) Bruce Vogelaar (Virginia Tech)

Long Baseline Neutrino Experiments Milind Diwan (BNL) Gina Rameika (Fermilab)

Neutrinoless Double-Beta Decay Steve Elliott (LANL) Charles Prescott (SLAC)

Nuclear Astrophysics and Underground Accelerators Joachim Goerres

(U. Notre Dame) Michael Wiescher

(U. Notre Dame)

Nucleon Decay/Atmospheric Neutrinos Chang Kee Jung (SUNY Stony Brook) Hank Sobel (UC Irvine)

Low-Background Counting Facilities and Prototyping Harry Miley (PNNL) Prisca Cushman (U. Minnesota)

Page 19: Deep Underground Science and Engineering Lab Hamish Robertson for the DUSEL S1 P/Is: E.W. Beier, C. Fairhurst, T.C. Onstott, R.G.H. Robertson, B. Sadoulet,

Other S1 Working GroupsDetermine the scientific reach of DUSEL

Rock Mechanics/Seismology Larry Costin (SNL) Paul Young (U. Toronto)

Applications Francois Heuzé (LLNL) Jean-Claude Roegiers (U. Oklahoma)

Coupled Processes Brian McPherson (New Mexico Tech) Eric Sonnenthal (LBNL)

Geomicrobiology Tommy Phelps (ORNL) Tom Kieft (New Mexico Tech)

Microbial Biology and Evolution Jim Fredrickson (PNNL) Nancy Moran (U. Arizona)

Infrastructure Requirements and Management Lee Petersen (CNA Engineers) Derek Ellsworth (Penn State U.) David Berley (U. Maryland)

Education and Outreach Willi Chinowski (LBNL) Susan Pfiffner (U. of Tennessee)