Overview and accomplishments of the Borexino experiment
نویسندگان
چکیده
منابع مشابه
Overview of the Borexino Solar Neutrino Experiment: the Physics and the Technical Requirements on Behalf of the Borexino Collaboration
In this paper an overview of the Borexino experiment will be give. The physics motivations and the background requirements are discussed.Furthermore, the main results from the Counting Test Facility of Borexino will be reported. The intention of this paper is to give answers to the following questions: \how are neutrinos measured in Borexino?", \why 7 Be neutrinos?" and \what can Borexino tell ...
متن کاملResults from the Borexino Experiment
Borexino is a low threshold liquid-scintillator detector for solar neutrinos located in the LNGS underground laboratory, Italy. Because of the ultra-high radio purity it is the first experiment able to do a real-time analysis of the low energetic solar neutrinos. A detection of the solar Be neutrinos with a rate of 49 ± 7 counts/day/100tons can be reported (192 days of live time measurement). B...
متن کاملStatus of the BOREXINO Solar Neutrino Experiment
Aim of BOREXINO is to measure in real time low energetic solar neutrinos via neutrino electron scattering. Special interest in BOREXINO is the measurement of the counting rate of the 861 keV 7 Be solar neutrinos in order to separate between scenarios beyond the standard model which are favored by the results of running solar neutrino experiments. The solar neutrino puzzle originates from the di...
متن کاملOverview and Accomplishments the SE/CM Perspective
The TIPSTER Architecture has been completed to the extent that the basic ~nctionality of components has been determined. Many interfaces, however, have not yet been defined to the level of detail which will be needed for the Government to meet its goals of software reuse and modular upgrading; i.e., they are under specified. The Architecture has been constructed with a high level of abstraction...
متن کاملWhich solar neutrino experiment after KamLAND and Borexino?
We estimate how well we will know the parameters of solar neutrino oscillations after KamLAND and Borexino. The expected error on ∆m is few per-mille in the VO and QVO regions, few per-cent in the LMA region, and around 10% in the LOW region. The expected error on sin 2θ is around 5%. KamLAND and Borexino will tell unambiguously which specific new measurement, dedicated to pp solar neutrinos, i...
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ژورنال
عنوان ژورنال: Journal of Physics: Conference Series
سال: 2016
ISSN: 1742-6588,1742-6596
DOI: 10.1088/1742-6596/675/1/012036