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1)Early Nu


3) Physics-Papers

3a)2013 posted Papers

4 a) DUSEL-Homestake

4 b) SURF

4 c) The SURF at Homestake


6)Other Expts.

7)Solar Neutrino Expt.

8)Reactor  Expt.-DAYABAY

9a) From BNL Neutrino News

9b) Murry News





13a)LBNE Collaboration
      Statement (Draft)

14) LBNE Monthly Reports

15 a) LBNF/ DUNE info

   b) LBNF/ DUNE News

Useful links



PDG Live




Alta Vista

NEW -- May 2014 -- NEW

* P5 Report,  S. Ritz to
HEPAP May 22, 2014 |click|

* Doon Gibbs, BNL Director's Statement on the Particle Physics Project Prioritization Panel (P5) Report to High Energy Physics Advisory Panel (HEPAP) May 22 |click|

* High Energy Physics Advisory Panel (HEPAP) Meeting, May 22-23, 2014, Maryland |click|


* Fourth "tau neutrino" was  Detected at the OPERA experiment, INFN Gran Sasso Lab, Italy, March 25, 2014: Muon Neutrino started at CERN, Geneva, after traveling 730 km through the Earth arrived at OPERA detector in Gran Sasso lab, transformed into "tau" neutrino, Their first "tau" neutrino was observed in 2010, second in 2012 and third in 2013, respectively.

*Electron Neutrino Appearance at the T2K Experiment Tsukuba, Japan, June 15, 2011: The T2K experiment, Detected 6 Electron Neutrino candidate...To continue Click: 1) T2K - KEK 2) T2K paper

*Fermilab on Electron Neutrino June 24, 2011,   click below: 1) |.html version| 2)|.text version|, 3) |plots|

Recent & Past Highlights

Dr. Zohreh Parsa Neutrino Physics, started CPV, LBN/LBNE studies in 1998. This page include part of her collaborative work. Dr.William Marciano Neutrino Physics, etc.; Awarded J. J. Sakurai Prize for Theoretical Particle Physics (2002) Dr. Nicholas Samios Early measurements of neutrino electron elastic scattering etc.;  Awarded Gian Carlo Wick Gold Medal   (2009) Dr. Raymond Davis Awarded 2002 Physics Nobel Prize for detecting Solar Neutrinos! Dr. Maurice Goldhaber
Experiment, revealed ν's to be left-handed, property known as "spin" Awarded National Medal of Science.
Dr. Melvin Schwartz Awarded Nobel Prize for Discovery of the Muon-Neutrino (1988).

Neutrino Physics & Experiment

Neutrino physics has had an interesting history. In 1930 Dr. Pauli postulated the existence of the (electron) neutrino, in 1956 this was confirmed by Drs. Reines and Cowan using a nuclear reactor source of antineutrinos. In 1962, a second distinct (muon) neutrino was shown to exist in a BNL experiment. For that discovery Nobel Prize was awarded to Drs. Lederman, Schwartz and Steinberger. In 1995, the third, (tau) neutrino was detected at FNAL. In parallel, Dr. Ray Davis' studies of solar neutrinos confirmed understanding of stellar dynamics modulo a 2/3 flux deficit that later was recognized as a result of ν oscillations among the three flavors of neutrinos. properties of those oscillations were further unveiled with followup solar, atmospheric, reactor and accelerator neutrino studies . The discovery of oscillations, detection
of 19 neutrino events from supernova 1987a by the old IMB and Kamiokande water cerenkov detectors confirmed the theory of supernova explosions. The WMAP experiment has started to see imprints of neutrino mass effects on the cosmic microwave background radiation left from the Big Bang.


In 1998 Dr. Zohreh Parsa started the Neutrino /CP Violation studies, that envisioned sending a very intense neutrino beam from Brookhaven National Laboratory on Long Island, New York through the earth to a (Long Baseline L, 1200 km < L < 4000 km) far away underground multipurpose large detector capable of: making precision measurements of all the (ν) neutrino oscillation parameters providing a major advance in ν science; search for proton decay; and observation of natural sources of neutrinos such as supernova.

The key to this approach is a very long distance. Length (L) of the Baseline defines the physics you can do,   once chosen, can not be changed without establishing a complete new facility.

By measuring muon neutrino disappearance and electron neutrino appearance, such a project would be capable of determining all 3 generation mixing angles, mass hierarchy, along with magnitude of the CP violation ( measuring CKM phase & explicitly observing differences in the muon neutrino and muon anti-neutrino oscillations). No existing experiment so far has such capability.

Very Long Baseline Neutrino Experiment

Using a wide band muon neutrino beam from BNL to a 2540 km underground ( 0.5 megaton water Cherenkov) detector at Homestake gold Mine in South Dakota was one of our first study for "very Long Baseline (underground detector) Neutrino Experiment" (LBNE).
Dr. Mann, U.Penn. was the first, (in person, phone calls, and messages persistently), to ask Dr. Parsa to consider the "Homestake Mine" (for her far away underground Detector site 2,540 km to BNL neutrino source).

He and others were interested in the results and worked hard to get funding for the Processing of the Homestake Mine. Drs. Marciano (2001), Kahn, McDonald (Princeton) and later Samios, others became interested in the (Extra) Very "Long Baseline Neutrino Experiment" (LBNE) that could search for CP violation in the lepton sector and precision studies of the neutrino mixing matrix and more.

Potentials of intense neutrino beams from BNL & FNAL to underground Detectors at Homestake, SD; Henderson and Cascades, WA were also studied as competition for Deep Underground Science and Engineering Laboratory Site increased. Later Homestake was selected.

Interest for LBNE in U.S. with neutrino source at BNL to a far Detector L=2540 km away at Homestake, S.D. grew. But after over a decade, possibility of LBNE with source at BNL became less likely, due to years of NSF/ and DOE funding delays, etc.     LBNE collaboration (Physics, Beam, Detector, etc., groups and studies with U.S. and International members) continued to grow.   Example of our earlier LBNE simulations are given below. Reload Firefox for more Figs. or if blank.

Fig.1 (Top Fig) Variation of parameters, e.g. variation of L (Baseline) distance from ν source to the detector, in Probability vs Energy plots. Fig.2 (Lower Fig) CP Phase Variations, in Probability vs Energy plots.

Fig. 3    Shows BNL, FNAL and 3 possible DUSEL Detector Sites, Homestake (SD), Henderson (CO), and Cascades (WA).

Fig. 4    Shows Super-Kamiokande is 50-kiloton water Cherenkov detector, filled with wate photomultiplier tubes (PMTs) on its walls.

LBNE (Reconfiguration) with ν source at FNAL

Using a high intensity accelerator neutrino beam from Fermilab (FNAL) to a (L=1287.475 km=800 miles baseline) liquid argon TPC detector at SURF (Homestake) is the LBNE reconfiguration. The goals for this program are determination of leptonic CP violation, the neutrino mass hierarchy, and underground physics.

On Dec 10, 2012, DOE granted Critical Decision 1 (CD-1) approval to the first phase of LBNE, which includes construction of a neutrino beamline at Fermilab (where the neutrino beam would travel through 800 miles of earth to a (near-surface) far detector at Sanford Lab in Lead, S.D. For Proposed LBNE Factsheet |click| For Brookhaven National Laboratory (BNL) DOE's approval of CD-1 was an important milestone after over decade of work.

May 22, 2014 - P5 Report recommended new international LBNF (Long Baseline Neutrino Facility), with FNAL as the host Lab, (see Left Tab for P5 Report, etc). Left Tabs provide more on LBNE with beam from FNAL to a Detecor at SURF; News, Reports etc.

March 2015 -- LBNE (Long Baseline Neutrino Experiment) was changed to ELBNF (Experiment at the Long-Baseline Neutrino Facility) at FNAL. ELBNF new spokespersons in E-mail thanked ELBNF/DUNE* (previously LBNE) collaboration, [*DUNE is a new name for: "Deep Underground Neutrino Experiment" ]. Information will be posted under Tab 15 "LBNF/ DUNE" ...  

Fig.5 BNL's Long Baseline Neutrino Experiment Team (May 2014)

Fig. 6    Drs. Z. Parsa, W. Marciano and R. Wilson in Henderson (Molybdenum Mine), was a proposed Underground Lab site in Co.

Neutrino (alias Neutrinos) updated: 1999-2014   Dr. Zohreh Parsa, Physics Dept. 510A, Brookhaven National Lab, Upton NY 11973.
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