Precision determination of invisible-particle masses at the CERN LHC. II.

Alan J. Barr, Alex Pinder, and Mario Serna
Phys. Rev. D 79, 074005 – Published 7 April 2009

Abstract

We further develop the constrained mass variable techniques to determine the mass scale of invisible particles pair-produced at hadron colliders. We introduce the constrained mass variable M3C which provides an event-by-event lower bound and upper bound to the mass scale given the two mass differences between the lightest three new particle states. This variable is most appropriate for short symmetric cascade decays involving two-body decays and on-shell intermediate states which end in standard-model particles and two dark-matter particles. An important feature of the constrained mass variables is that they do not rely simply on the position of the end point but use the additional information contained in events which lie far from the end point. To demonstrate our method we study the supersymmetric model SPS 1a. We select cuts to study events with two χ˜2o each of which decays to χ˜1o, and two opposite-sign same-flavor charged leptons through an intermediate on-shell slepton. We find that with 300fb1 of integrated luminosity the invisible-particle mass can be measured to Mχ˜1o=96.4±2.4GeV. Combining fits to the shape of the M3C constrained mass variable distribution with the maxmll edge fixes the mass differences to ±0.2GeV.

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  • Received 1 December 2008

DOI:https://doi.org/10.1103/PhysRevD.79.074005

©2009 American Physical Society

Authors & Affiliations

Alan J. Barr1,*, Alex Pinder1,†, and Mario Serna2,‡

  • 1Department of Physics, Denys Wilkinson Building, University of Oxford, Keble Road, Oxford OX1 3RH, United Kingdom
  • 2Rudolf Peierls Centre for Theoretical Physics, University of Oxford, Keble Road, Oxford, OX1 3NP, United Kingdom

  • *a.barr@physics.ox.ac.uk
  • a.pinder1@physics.ox.ac.uk
  • mariojr@alum.mit.edu

See Also

Precision determination of invisible-particle masses at the CERN LHC

Alan J. Barr, Graham G. Ross, and Mario Serna
Phys. Rev. D 78, 056006 (2008)

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Vol. 79, Iss. 7 — 1 April 2009

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