Deep Science at Boulby Underground Laboratory: [PDF]

Large Expt. Cave Area: Internal lab height/ width of 6.5m/7m. Offices &. People. Entrance. Materials. Entrance 1. Ma

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Idea Transcript


Deep Science at Boulby Underground Laboratory:

Factor ~1 million reduction in cosmic ray muon flux vs. surface

Boulby Geology

Typical Boulby Salt Roadway Boulby Mine

Mine Sha)s Rock-Salt

Potash

Palmer Lab

Mining at Boulby…

•  DRIFT: Directional Dark Matter Search •  BUGs: Ultra-low background material screening •  Deep Carbon: Muon Tomography for CCS (etc) •  ERSaB: Environmental gamma spectroscopy •  BISAL: Geomicrobiology / Astrobiology studies •  MINAR: Space Exploration Tech. Development •  Misc. Geology / Geoscience •  Misc. Low-background support projects •  Etc... (More to come). A growing mulC-disciplinary science programme: from astrophysics (Dark MaIer) to studies of geology, climate, the environment, life on Earth and beyond.

DRIFT-II

Ÿ Supports work of 9 collaboraCve projects (astrophysics to climate, geology, environment, life etc), 20 insCtuCons, > 70 scienCsts and students. •  Facility funded and operated by the Science and Technology FaciliCes Council (STFC) in partnership with CPL/ICL.

Environment monitoring Management

•  OperaCons, H&S & science programme managed by 4(+3) onsite staff and supported by Rutherford Appleton Lab (PPD).

H&S, medical support

•  CPL / ICL provide wide-ranging operaConal & higher level support. ‘A hole in the ground does not make a facility’

User and science support

Materials transport

Project tracking, H&S

A NEW LABORATORY now being built at Boulby New Laboratory To replace current facility and host planned & new construc>on plan projects for the next decade and more…

Mars Analogue Area & outside tesCng area

Project comple>on date: End 2016

Materials Entrance 2

Main hall: Internal Lab height/width of 4m/7m

Materials Entrance 1

Palmer lab Offices & People Entrance

Large Expt. Cave Area: Internal lab height/ width of 6.5m/7m 50m

BUGS ULB CounCng facility

Material Store

Fully-equipped 4000m3 lab. Class 10K & 1K clean room throughout. 5-10T li)ing capacity.

New Laboratory Details 10T and 5T Gantry cranes

Ouhiing: Power, gas & fire detecCon, IT / comms, AC & filtraCon

Raised Steel floor

Large Experimental Cavern (6mx7m Internal HxW) Main Hall (4mx7m internal HxW)

Steel frame throughout. 1m spacing

Expected compleCon July 2016

‘BUGS’ ULB Germanium Facility

Main Experimental Hall (7x4x60m)

Boulby New Lab ConstrucCon March 2016 > 4000m3 of well supported class 1,000 and class 10,000 clean room experimental space

Large Experimental Cavern (LEC) (7x7x35m)

Air condiConing, HEPA filtraCon, internet / comms, 5 & 10 Tonne li)ing capacity.

CompleCon Jan/Feb 2016

Now moving experiments in from old lab.

Boulby New Lab Large Experimental Cavern (LEC) July 2016

ULB Material Screening

S.M.Paling - [email protected]

SURF Lab and LZ project management team visit to Boulby Ge Suite – Aug 2015

Boulby has hosted Dark MaIer search studies for two decades. Including the NAIAD, DRIFT & ZEPLIN experiment programmes. Boulby now hosts DRIFT DirecConal DM programme, doing R&D for DM-Ice & providing ULB material screening for other studies, inc LUX-ZEPLIN Alpha

ZEPLIN-III @ Boulby

DM-Ice

ZEPLIN: The world’s first 2-phase Xenon dark maCer detector (Finished 2011) DRIFT-IId

Current limits & future projecCons

A

Dark MaIer Detector.

STATUS: Programme operaCng at Boulby since 2001. Currently limit-seing and conducCng system performance & scale-up R&D. Plans for further R&D & expansion / collaboraCon (CYGNUS). Rotation of visible matter WITHIN the Dark Matter halo

Dual (1m3 total) NegaCve Ion DRIFT TPC DirecConal detecCon

Tvis~240Myrs

Alpha track

Vsun~230kms-1 Dark matter Halo

WIMP Wind

Directional DM detection – providing the most powerful direct detection signature

DRIFT-IId @ Boulby

Occidental College, New Mexico, Colorado State, Hawaii, Wellesley, Sheffield, Edinburgh, Boulby

Growing suite (‘BUGS’) of Ultra-Low-Background germanium detector systems to support Dark Matter & misc ‘rare-event’ studies… Activity testing steel samples

Ortec

Background Spectra

Ÿ Ortec 2kg Coax (90% eff). Ÿ 2 Canberra BEGe detectors Ÿ Canberra SAGe Well-type

Ultra Low background counting studies supporting UK DM (LZ) & 0nuBB communities.

Sensitivity down to al for cheap, reliable, prac>cal, real->me long-term monitoring of deep structures. Poten>al applica>ons: -  Deep geological repository monitoring. -  Monitoring in Carbon Capture & Storage (CCS)

Muon-Cdes detector development

Bore hole detector installaCon

CCS site simulaCon

Deep-Carbon Project: £1.4M funding from UK Dept of Energy & Climate change (DECC) & Premier Oil: Ÿ Bore-hole detector development & tesCng @ Boulby Ÿ Muon-Tides technology demonstrator Ÿ SimulaCons of technique performance in CCS



A base for studies of life in Boulby rock – studies of limits of Sampling life in Boulby Subsurface Astrobiology Laboratory Brine life on earth and on Led by Edinburgh, other planets ALSO: An important ‘Mars Analogue site’ UKCA – with geology & conditions to allow explorations & astrobiology technique & instrumentation development Mining & extraplanetary exploration instrumentation development

MINAR 2

Life in Boulby salt

Boulby New Lab: Outside Experimenta>on Area

Under construcCon…

Large Experimental Cavern (LEC)

Open salt (etc) roadways support & equipped for easy experiment access

Misc Geology / Geoscience Durham, Imperial College, Boulby, Edinburgh BriYsh Geological Survey (BGS)

Misc. geology & geoscience studies @ Boulby. Improved mining technologies E.g. enhanced extraction but reduced subsidence? Rock deformation studies E.g. salt deformation and oil reservoirs? Seismology E.g. how does stress change induce earthquakes? Carbon Capture & Storage E.g. The effect of fractures on the sealant properties of anhydrite for CCS Geochemistry E.g. how does fluid (oil) move through rock masses? Geomicrobiology E.g. What effect do microbes of rock stuctural integrity (cliff, geological repositories)

Micro-seismic monitoring

Subsidence mapping

Geochemistry Cliff erosion mapping

Funding past and present: One NE, CPL / ICL NERC, Crown Estate Anhydrite mechanical properCes



We need you to tell us how to maximise the potenCal for our lab to support your type of work

Come and visit!

Boulby Underground Laboratory Review of expressions of interest Coming Soon (early 2017)

Thank You…. .

Come and visit / work-with us… Email: [email protected] Web: www.stfc.ac.uk/boulby Emma Meehan STFC Boulby Underground Science Facility

Facebook: Boulby Underground Laboratory

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