Solving the Solar Neutrino Problem 2 Km Underground — the Sudbury Neutrino Observatory

نویسنده

  • A. W. P. POON
چکیده

The Sudbury Neutrino Observatory (SNO) is capable of measuring simultaneously the flux of electron-type neutrinos and the total flux of all active flavours of neu-trinos originating from the Sun. A model-independent test of neutrino flavour transformation was performed by comparing these two measurements. Assuming an undistorted neutrino energy spectrum, this transformation has been definitively demonstrated in the pure D 2 O phase of the SNO experiment. In the second phase with dissolved NaCl in the D 2 O, the total active solar neutrino flux was measured without any assumption on the energy dependence of flavour transformation. In this talk, results from these measurements, their physics implications and the current status of the SNO experiment are presented.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Sudbury Neutrino Observatory Results

A. B. McDonald Physics Department Queen's University Kingston, Ontario CANADA K7L 3N6 For the SNO Collaboration e-mail [email protected] Abstract The Sudbury Neutrino Observatory uses 1000 tonnes of heavy water in an ultraclean Cherenkov detector situated 2 km underground in Ontario, Canada to study neutrinos from the Sun and other astrophysical sources. The Charged Current (CC) reaction on deuteri...

متن کامل

The Sudbury Neutrino Observatory

The Sudbury Neutrino Observatory is a second-generation water Cherenkov detector designed to determine whether the currently observed solar neutrino de"cit is a result of neutrino oscillations. The detector is unique in its use of D 2 O as a detection medium, permitting it to make a solar model-independent test of the neutrino oscillation hypothesis by comparison of the chargedand neutral-curre...

متن کامل

Results from the Neutral Current Detector phase of the Sudbury Neutrino Observatory

The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector designed to solve the long-standing “solar neutrino problem”; a discrepancy between the measured and predicted flux of electron-flavour solar neutrinos. SNO measured the rate of charged-current and neutral-current reactions of neutrinos in heavy water and was able to demonstrate that neutrinos from the Sun, produced in t...

متن کامل

Model-Independent Measurement of the Neutral-Current Interaction Rate of Solar 8B Neutrinos with Deuterium in the Sudbury Neutrino Observatory

Model-Independent Measurement of the Neutral-Current Interaction Rate of SolarB Neutrinos with Deuterium in the Sudbury Neutrino Observatory by Karsten Miklas Heeger Chair of Supervisory Committee:Professor R.G. Hamish RobertsonPhysics With heavy water as a target medium the Sudbury Neutrino Observatory (SNO) is de-signed to study solar neutrinos by measuring both the total flux...

متن کامل

Neutrinos in Stochastic Media: From Sun to Core-Collapse Supernovae

Recent work on neutrino propagation in stochastic media and its implications for the Sun and corecollapse supernovae are reviewed. It is shown that recent results from Sudbury Neutrino Observatory and SuperKamiokande combined with a best global fit value of δm2 = 5× 10−5 eV2 and tan2 θ = 0.3 rule out solar electron density fluctuations of a few percent or more. It is argued that solar neutrino ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2003