Linda M. Carpenter
Santa Cruz Institute for Particle Physics
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Featured researches published by Linda M. Carpenter.
Physical Review D | 2009
Linda M. Carpenter; Michael Dine; Guido Festuccia; John D. Mason
Recently there has been much progress in building models of gauge mediation, often with predictions different than those of minimal gauge mediation. Meade, Seiberg, and Shih have characterized the most general spectrum which can arise in gauge-mediated models. We discuss some of the challenges of building models of general gauge mediation, especially the problem of messenger parity and issues connected with R symmetry breaking and CP violation. We build a variety of viable, weakly coupled models which exhibit some or all of the possible low energy parameters.
Physical Review D | 2013
Linda M. Carpenter; Daniel Whiteson; Tim M. P. Tait; A. Nelson; Chase Owen Shimmin
Searches for dark matter at colliders typically involve signatures with energetic initial-state radiation without visible recoil particles. Searches for mono-jet or mono-photon signatures have yielded powerful constraints on dark matter interactions with Standard Model particles. We extend this to the mono-Z signature and reinterpret an ATLAS analysis of events with a Z boson and missing transverse momentum to derive constraints on dark matter interaction mass scale and nucleon cross sections in the context of effective field theories describing dark matter which interacts via heavy mediator particles with quarks or weak bosons.
Physical Review D | 2009
Linda M. Carpenter; Michael Dine; Guido Festuccia; Lorenzo Ubaldi
In supersymmetric theories, the presence of axions usually implies the existence of a noncompact, (pseudo)moduli space. In gauge-mediated models, the axion would seem a particularly promising dark matter candidate. The cosmology of the moduli then constrains the gravitino mass and the axion decay constant; the former cannot be much below 10 MeV; the latter cannot be much larger than 10{sup 13} GeV. Axinos, when identifiable, are typically heavy and do not play an important role in cosmology.
Physical Review D | 2014
A. Nelson; Linda M. Carpenter; Randel Cotta; Adam Johnstone; Daniel Whiteson
We describe an effective theory of interaction between pairs of dark matter particles and pairs of photons. Such an interaction could accomodate
Journal of High Energy Physics | 2011
Linda M. Carpenter
\chi\bar{\chi}\rightarrow\gamma\gamma
Physical Review D | 2017
Linda M. Carpenter; Tao Han; Khalida Hendricks; Zhuoni Qian; N. Zhou
processes which might be the cause of the observed feature in the FermiLAT spectrum, as well as
Physical Review D | 2015
Linda M. Carpenter; Russell Colburn; Jessica Goodman
\gamma^*/Z\rightarrow \gamma\chi\bar{\chi}
Physical Review D | 2014
Linda M. Carpenter; Daniel Whiteson; Anthony DiFranzo; M. Mulhearn; Sean Tulin; Chase Owen Shimmin
processes, which would predict excesses at the LHC in the
arXiv: High Energy Physics - Phenomenology | 2008
Linda M. Carpenter
\gamma+\missET
arXiv: High Energy Physics - Phenomenology | 2005
Linda M. Carpenter; Patrick J. Fox; David E. Kaplan
final-state. We reinterpret an ATLAS