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Re: sno
- To: Peter Kammel <kammel@npl.uiuc.edu>
- Subject: Re: sno
- From: Bernhard Lauss <lauss@berkeley.edu>
- Date: Wed, 30 Nov 2005 16:00:33 -0800 (PST)
- In-reply-to: <Pine.LNX.4.21.0511171406040.7920-100000@one.npl.uiuc.edu>
- References: <Pine.LNX.4.21.0511171406040.7920-100000@one.npl.uiuc.edu>
dear Peter,
In the recent PRC issue
Phys. Rev. C 72, 055502 (2005)
page 33 of the paper,
SNO improved to 5.5 experimental error
still much larger thatn 1.1 cross section
http://scitation.aip.org/getabs/servlet/GetabsServlet?prog=normal&id=PRVCAN000072000005055502000001&idtype=cvips&gifs=Yes&type=ALER
Bernhard
*******************************************************************
Bernhard Lauss E-Mail: lauss@socrates.berkeley.edu
Physics Department
366 LeConte Hall
University of California @ Berkeley
Berkeley, CA 94720 Tel: (510)-642 4057
United States Fax: (510)-642 9811
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On Thu, 17 Nov 2005, Peter Kammel wrote:
> Dear Fred, dear Bernhard,
>
> MEASUREMENT OF THE TOTAL ACTIVE B-8 SOLAR NEUTRINO FLUX AT THE SUDBURY
> NEUTRINO OBSERVATORY WITH ENHANCED NEUTRAL CURRENT SENSITIVITY.
> By SNO Collaboration (S.N. Ahmed et al.). Sep 2003. 5pp.
> Published in Phys.Rev.Lett.92:181301,2004
> e-Print Archive: nucl-ex/0309004
>
> gives NC flux CC flux
> total exp uncertainty +-7.3 -4.6,+3.8
> x-section uncertainty +-1.1 +-1.2
>
> The x-section uncertainty mainly relies on the Kubodera calc using
> the tritium constraint. But the exp uncertainties are significant.
> I don't know if SNO will be able to improve on that.
>
> Regards
>
> Peter
>
>