J un 1 99 4 Neutrino Oscillations in Noisy Media

نویسندگان

  • F. N. Loreti
  • A. B. Balantekin
چکیده

We develop the Redfield equation for delta-correlated gaussian noise and apply it to the case of two neutrino flavor or spin precession in the presence of a noisy matter density or magnetic field, respectively. The criteria under which physical fluctuations can be well approximated by the delta-correlated gaussian noise for the above cases are examined. Current limits on the possible neutrino magnetic moment and solar magnetic field suggest that a reasonably noisy solar magnetic field would not appreciably affect the solar electron neutrino flux. However, if the solar electron density has fluctuations of a few percent of the local density and a small enough correlation length, the MSW effect is suppressed for a range of parameters.

برای دانلود 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

X iv : h ep - p h / 97 06 23 9 v 1 4 J un 1 99 7 Does the Sun Appear Brighter at Night in Neutrinos ?

We calculate accurately the number of solar neutrino events expected as a function of solar zenith angle, with and without neutrino oscillations, for detectors at the locations of Super-Kamiokande, SNO, and the Gran Sasso National Laboratory. Using different earth models to estimate geophysical uncertainties, and different solar models to estimate solar uncertainties, we evaluate distortions pr...

متن کامل

ar X iv : h ep - p h / 99 05 48 3 v 1 2 6 M ay 1 99 9 McGill - 99 / 20 NEUTRINO PROPAGATION THROUGH FLUCTUATING MEDIA

The description of neutrino propagation through a fluctuating medium is summarized. Fluctuation-Dissipation-Theorem arguments relate microscopic fluctuations to thermodynamic quantities, allowing these to be very generally studied in astro-physical environments. Fluctuation-induced modifications to neutrino oscillations have been studied in detail within the Sun and within the envelope of super...

متن کامل

ar X iv : h ep - p h / 99 10 24 6 v 2 7 O ct 1 99 9 UH - 511 - 941 - 99 September 1999 Neutrino Anomalies without Oscillations ∗

I review explanations for the three neutrino anomalies (solar, atmospheric and LSND) which go beyond the “conventional” neutrino oscillations induced by mass-mixing. Several of these require non-zero neutrino masses as well.

متن کامل

Neutrino oscillations in noisy media.

We develop the Reddeld equation for delta-correlated gaussian noise and apply it to the case of two neutrino avor or spin precession in the presence of a noisy matter density or magnetic eld, respectively. The criteria under which physical uctuations can be well approximated by the delta-correlated gaussian noise for the above cases are examined. Current limits on the possible neutrino magnetic...

متن کامل

Neutrino Oscillations with Four Generations

There have been several experiments 10,11,12,13 which suggest neutrino oscillations. To explain the solar, atmospheric and LSND data within the framework of neutrino oscillations, it is necessary to have at least four kinds of neutrinos. It has been shown in the two flavor framework that the solar neutrino deficit can be explained by neutrino oscillation with the sets of parameters (∆m⊙, sin 2 ...

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

برای دانلود 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

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008