Difference between revisions of "Data Rates"

Jump to navigation Jump to search
Line 44: Line 44:
== References ==
== References ==
* [http://arxiv.org/abs/hep-ph/0407297 Very massive underground detectors for proton decay searches]
* [http://arxiv.org/abs/hep-ph/0407297 Very massive underground detectors for proton decay searches]
* [https://indico.fnal.gov/getFile.py/access?contribId=3&resId=3&materialId=slides&confId=9209 PDK at LBNF Meeting in Jan'15]
= Solar =
= Solar =

Revision as of 15:09, 16 April 2015


This page is in initial stages of construction.


According to the physics goals of the experiment, we need to consider the following main sources of signal:

  • The "beam neutrino" signal
  • The Supernova Burst (SNB) signal
  • Proton Decay
  • Solar neutrinos

All these signals have distinct energy scales, topologies and other characteristics. In terms of buffering and processing data in real or near time, they pose different requirements.

Beam Neutrinos

Because of the energy scale (~GeV range) neutrino interactions will be characterized by TPC signals well above radiological background. Zero-suppression will lead to significant reduction of data volume and rates (the detector will appear "empty" for the most part).



νe+40Ar ⇒ e-+40K*

ν e+40Ar ⇒ e++40Cl*

νx+40Ar ⇒ νx+40Ar*

νe,x+e- ⇒ νe,x+e-



  • DocDB 6977 - Software for low-energy signals
  • DocDB 8481 - Summary of SNB Working Group Progress (February 2014)

Some reference curves from DocDB 6977:

SNB spectrum 1.png

In a nutshell:

  • approximately 100 events per kiloton, spread over ~30 seconds, ~½ in first second
  • all flavors, few tens of MeV

Other material

Proton Decay




  • DocDB 6212 - M.Smy's slides from 2012 (LBNE solar studies potential)


Background Sources


Important radiologicals

  • 39Ar 1.01 Bq/kg β- End-point: 0.565MeV
  • 85Kr 0.1-0.3 Bq/kg β- End-point: 0.687MeV


Muon and Neutron Backgrounds (40Cl)

Solar bkg 1.png

Summary Plots

Caveat - in the plots below the neutron data reflect the number of neutrons, not tracks, hits or counts created by neutrons. TBD! BGRates.png

Same plot, but in large (5MeV) bins:
BGRates 5MeVBins.png