It was designed to be a low-cost, low-maintenance detector[5] with limited capabilities[6]: 38 sufficient for the burst of neutrinos generated by a nearby supernova. Its major components are left over from other decommissioned experiments: 76 tons of lead from an earlier cosmic-ray experiment, and 128 three-metre-long helium-3neutron detectors from the Sudbury Neutrino Observatory.
The idea of using lead to detect supernova neutrinos was originally proposed in 1996 by Cliff Hargrove as the "lead astronomical neutrino detector" (LAND),[7] and in 2004, Charles Duba, then a PhD student working on SNO, proposed re-using them for this purpose, prompting the renaming to HALO. Design of the current detector began in 2007.[2]
When an electron neutrino collides with a lead nucleus, it causes a nuclear transmutation that ends with a neutron emission. Lead does not absorb neutrons readily since 208Pb it has a "magic number" of both protons and neutrons, so the neutrons pass through to the 3He detectors. If enough neutrons are detected in a short time, an alert is generated.
One limitation of the detector's design is its small size; due to the limited amount of surplus lead available, half of the neutrons generated escape before hitting a neutron detector.[5]: 15 To mitigate this, it is surrounded by a layer of water to reflect some of the neutrons back in. Budget permitting, there are plans for a larger detector using 1000 t of lead and the remaining leftover 3He detectors[5]: 13–18 (Due to lead's high density; 1000 t is a cube 4.45 m (14.6 ft) on a side, not an impractical size for underground installation.)
References
^Duba, C A; Duncan, F; Farine, J; Habig, A; Hime, A; Robertson, R G H; Scholberg, K; Shantz, T; Virtue, C J; Wilkerson, J F; Yen, S (1 November 2008). "HALO – the helium and lead observatory for supernova neutrinos". Journal of Physics: Conference Series. 136 (4): 042077. Bibcode:2008JPhCS.136d2077D. doi:10.1088/1742-6596/136/4/042077.
^ abScholberg, Kate (2012-05-09). "HALO is running!". Duke Neutrino Group blog. Retrieved 2014-11-22.
^"HALO experiment joins SuperNovae Early Warning System" (Press release). SNOLAB. 2015-10-16. Retrieved 2015-12-06. The HALO supernova neutrino detector in SNOLAB has joined the international SuperNova Early Warning System (SNEWS).
^"SNEWS News". Retrieved 2015-12-06. December 2015: HALO joins SNEWS, bringing total to 7 experiments.
^ abcVirtue, C.J. (22–23 August 2007). HALO: a Helium and Lead Observatory. SNOLAB Workshop VI. Sudbury.
^Yen, Stanley (19 July 2012). Helium And Lead Observatory for supernova neutrinos(PDF). Core-Collapse Supernovae: Models and Observable Signals. Sudbury. (There is a video of the talk at the conference page.)
^Hargrove, C.K.; Batkin, I.; Sundaresan, M.K.; Dubeau, J. (August 1996), "A lead astronomical neutrino detector: LAND", Astroparticle Physics, 5 (2): 183–196, Bibcode:1996APh.....5..183H, doi:10.1016/0927-6505(96)00019-9
helium, lead, observatory, helium, lead, observatory, halo, neutrino, detector, snolab, supernova, early, warning, system, snews, began, engineering, operation, 2012, joined, operational, part, snews, october, 2015, designed, cost, maintenance, detector, with,. The Helium And Lead Observatory HALO is a neutrino detector at SNOLab for the Supernova Early Warning System SNEWS 1 It began engineering operation on May 8 2012 2 and joined as an operational part of SNEWS in October 2015 3 4 It was designed to be a low cost low maintenance detector 5 with limited capabilities 6 38 sufficient for the burst of neutrinos generated by a nearby supernova Its major components are left over from other decommissioned experiments 76 tons of lead from an earlier cosmic ray experiment and 128 three metre long helium 3 neutron detectors from the Sudbury Neutrino Observatory The idea of using lead to detect supernova neutrinos was originally proposed in 1996 by Cliff Hargrove as the lead astronomical neutrino detector LAND 7 and in 2004 Charles Duba then a PhD student working on SNO proposed re using them for this purpose prompting the renaming to HALO Design of the current detector began in 2007 2 When an electron neutrino collides with a lead nucleus it causes a nuclear transmutation that ends with a neutron emission Lead does not absorb neutrons readily since 208Pb it has a magic number of both protons and neutrons so the neutrons pass through to the 3He detectors If enough neutrons are detected in a short time an alert is generated One limitation of the detector s design is its small size due to the limited amount of surplus lead available half of the neutrons generated escape before hitting a neutron detector 5 15 To mitigate this it is surrounded by a layer of water to reflect some of the neutrons back in Budget permitting there are plans for a larger detector using 1000 t of lead and the remaining leftover 3He detectors 5 13 18 Due to lead s high density 1000 t is a cube 4 45 m 14 6 ft on a side not an impractical size for underground installation References Edit Duba C A Duncan F Farine J Habig A Hime A Robertson R G H Scholberg K Shantz T Virtue C J Wilkerson J F Yen S 1 November 2008 HALO the helium and lead observatory for supernova neutrinos Journal of Physics Conference Series 136 4 042077 Bibcode 2008JPhCS 136d2077D doi 10 1088 1742 6596 136 4 042077 a b Scholberg Kate 2012 05 09 HALO is running Duke Neutrino Group blog Retrieved 2014 11 22 HALO experiment joins SuperNovae Early Warning System Press release SNOLAB 2015 10 16 Retrieved 2015 12 06 The HALO supernova neutrino detector in SNOLAB has joined the international SuperNova Early Warning System SNEWS SNEWS News Retrieved 2015 12 06 December 2015 HALO joins SNEWS bringing total to 7 experiments a b c Virtue C J 22 23 August 2007 HALO a Helium and Lead Observatory SNOLAB Workshop VI Sudbury Yen Stanley 19 July 2012 Helium And Lead Observatory for supernova neutrinos PDF Core Collapse Supernovae Models and Observable Signals Sudbury There is a video of the talk at the conference page Hargrove C K Batkin I Sundaresan M K Dubeau J August 1996 A lead astronomical neutrino detector LAND Astroparticle Physics 5 2 183 196 Bibcode 1996APh 5 183H doi 10 1016 0927 6505 96 00019 9External links Edithttp www snolab ca halo Coordinates 46 28 19 N 81 11 12 W 46 4719 N 81 1866 W 46 4719 81 1866 Retrieved from https en wikipedia org w index php title Helium and Lead Observatory amp oldid 1014585414, wikipedia, wiki, book, books, library,
