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Group NEUTRINOS AND DARK MATTER EXPERIMENTS. NEUTRINO AND DARK MATTER EXPERIMENTS AT BERKELEY. Cleaning the MiniCLEAN vessel. Boating in the acrylic vessel during SNO. PSUP: the SNO PMT support structure. SNO cavity and PMT support structure. View of the cavity that will house MiniCLEAN. Container for the MiniCLEAN experiment. Brianna, a Berkeley undergrad, poses with the MiniCLEAN vessel. Sudbury's (in)famous big nickel. Nov 10, 2015: ARTHUR MCDONALD GIVES A TALK ABOUT SNO AT THE BERKELEY LAB. Oct 6, 20...

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Group NEUTRINOS AND DARK MATTER EXPERIMENTS. NEUTRINO AND DARK MATTER EXPERIMENTS AT BERKELEY. Cleaning the MiniCLEAN vessel. Boating in the acrylic vessel during SNO. PSUP: the SNO PMT support structure. SNO cavity and PMT support structure. View of the cavity that will house MiniCLEAN. Container for the MiniCLEAN experiment. Brianna, a Berkeley undergrad, poses with the MiniCLEAN vessel. Sudbury's (in)famous big nickel. Nov 10, 2015: ARTHUR MCDONALD GIVES A TALK ABOUT SNO AT THE BERKELEY LAB. Oct 6, 20...

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7 group site

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9 chess experiment

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OG Group Web | underground.physics.berkeley.edu Reviews

https://underground.physics.berkeley.edu

Group NEUTRINOS AND DARK MATTER EXPERIMENTS. NEUTRINO AND DARK MATTER EXPERIMENTS AT BERKELEY. Cleaning the MiniCLEAN vessel. Boating in the acrylic vessel during SNO. PSUP: the SNO PMT support structure. SNO cavity and PMT support structure. View of the cavity that will house MiniCLEAN. Container for the MiniCLEAN experiment. Brianna, a Berkeley undergrad, poses with the MiniCLEAN vessel. Sudbury's (in)famous big nickel. Nov 10, 2015: ARTHUR MCDONALD GIVES A TALK ABOUT SNO AT THE BERKELEY LAB. Oct 6, 20...

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underground.physics.berkeley.edu

1

OG Group Web

http://underground.physics.berkeley.edu/SNO+.html

Group NEUTRINOS AND DARK MATTER EXPERIMENTS. Neutrino-less double beta decay. Liquid scintillator is an organic liquid that gives off light when charged particles pass through it. SNO will detect neutrinos when they interact with electrons in the detector to produce charged particles which, in turn, create light as they pass through the scintillator. The flash of light is then detected by the PMT array, and is converted into information such as energy and position of the particle. Several test setups in ...

2

OG Group Web

http://underground.physics.berkeley.edu/MiniCLEAN.html

Group NEUTRINOS AND DARK MATTER EXPERIMENTS. The DEAP/CLEAN focus is on purely liquid detectors, also called "single-phase" detectors, rather than combination liquid gas detectors, and specifically on Ar and Ne. The simplicity of a liquid-only detector, and the relatively low cost of argon and neon, make it practical and inexpensive to scale the technology up to 50 tonne targets with minimal R&D. Detector construction and commissioning. Vacuum ultra violet R&D. Tetraphenyl Butadiene (TPB) is a commonly u...

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http://underground.physics.berkeley.edu/gallery.html

Group NEUTRINOS AND DARK MATTER EXPERIMENTS.

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OG Group Web

http://underground.physics.berkeley.edu/chess.html

Group NEUTRINOS AND DARK MATTER EXPERIMENTS. An immediate clear advantage of this new technology is adding the directionality information in a scintillation detector. This is specially interesting in neutrino-less double beta decay experiment (LINK) like SNO , where the main background is composed by the solar neutrino events and resolving the direction of these events would help to reduce events coming from the sun. Cherenkov and Scintillation separation. Admixtures of linear-alkybencene (LAB) mixed wit...

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OG Group Web

http://underground.physics.berkeley.edu/news.html

Group NEUTRINOS AND DARK MATTER EXPERIMENTS. Nov 10, 2015: ARTHUR MCDONALD GIVES A TALK ABOUT SNO AT THE BERKELEY LAB. Nov 9, 2015: SNO AWARDED WITH THE BREAKTHROUGH PRIZE OF PHYSICS. Oct 6, 2015: ARTHUR MCDONALD, NOBEL PRIZE IN PHYSICS 2015. Arthur B. McDonald, director of SNOLAB and SNO collaborator, awarded with the 2015 Nobel Prize in Physics for the discovery of neutrino oscillation at the SNO detector, showing neutrinos are massive particles. The prize is shared with Takaaki Kajita for the ...After...

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cosmology.lbl.gov

Berkeley Cosmology Group Directory

http://cosmology.lbl.gov/directory.html

Berkeley Cosmology Group Directory. E-mail addresses should be appended by berkeley.edu or .gov, for lbl addresses, if address is incomplete. Long term (faculty and research staff). Shorter term: Postdocs, Visitors. Long term (faculty and research staff). CMB Experiment and Data Analysis. Computational Cosmology Center LBL, (510) 486-7308, jdborrill@lbl.gov. 433 LeConte, 642-5036, UCB Physics faculty, swlh@cosmology.berkeley.edu, link. Computational Cosmology Center, (510) 495-2697,tskisner@lbl.gov.

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OG Group Web

Group NEUTRINOS AND DARK MATTER EXPERIMENTS. NEUTRINO AND DARK MATTER EXPERIMENTS AT BERKELEY. Cleaning the MiniCLEAN vessel. Boating in the acrylic vessel during SNO. PSUP: the SNO PMT support structure. SNO cavity and PMT support structure. View of the cavity that will house MiniCLEAN. Container for the MiniCLEAN experiment. Brianna, a Berkeley undergrad, poses with the MiniCLEAN vessel. Sudbury's (in)famous big nickel. Nov 10, 2015: ARTHUR MCDONALD GIVES A TALK ABOUT SNO AT THE BERKELEY LAB. Oct 6, 20...

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