Re: APS Neutrino Study: Reactor Working Group

Dear Gabriela and Ed,

     We with Sandhya Choubey could write the part concerning the
  Physics possibilities of a reactor neutrino experiments
to determine the solar neutrino oscillation parameters
(delta m_12, theta_12). Let us know
your opinion.

                  With best regards,

                           Serguey Petcov

On Mon, 16 Feb 2004, Gabriela Barenboim wrote:

> Dear Colleagues,
> Here is an updated outline for our working group report.
> Please contact us if you would like to contribute to a particular
> section. During the next week, we will begin contacting people to
> make first drafts of particular sections.
> Best wishes,
> Gabriela and Ed
> -------------------------------------------------------------------------------
>
> (0) Overview -- Brief history of reactor experiments
> * Chooz & Palo Verde
> * KamLAND
>
>
> (I) Physics possibilities of a reactor neutrino experiment
>
> * theta_13
> * solar physics (delta m_12, theta_12)
> * sin2 theta_w
> * supernova
> * CPT
> * neutrino magnetic moments
>
>
> (II) (A) The theta_13 experiment
>
> * General strategies to improve CHOOZ
>
> * Issues relevant for evaluating the experiments
> efficiency
> background
> reactor power
>
> * Different scales of experiment
>
> small
> medium
> large
> (For each: describe strategy of experiment, justify theta_13
> sensitivity, give rough timescale/cost)
>
> (B) Complementarity with accelerators
>
> (III) Beyond theta_13
> * sin2 theta_w
> * supernova
> * Deltam_12
> * CPT
>
> (IV) Conclusions
>
Received on Tue Feb 17 03:11:15 2004