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Theoretical physicists working at a blackboard collaboration pod in the Beecroft building.
Credit: Jack Hobhouse

John March-Russell

Professor of Theoretical Physics and Senior Research Fellow, New College, Oxford; Perimeter Institute Distinguished Visiting Research Chair

Research theme

  • Particle astrophysics & cosmology
  • Fundamental particles and interactions
  • Fields, strings, and quantum dynamics

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Particle theory
  • AION/Magis
John.March-Russell@physics.ox.ac.uk
Telephone: 01865 (2)73630
Rudolf Peierls Centre for Theoretical Physics, room 60.05
  • About
  • Publications

Baryogenesis via Particle-Antiparticle Oscillations

(2016)

Authors:

Seyda Ipek, John March-Russell
More details from the publisher

Natural Scherk-Schwarz theories of the weak scale

Journal of High Energy Physics Springer Nature 2015:12 (2015) 1-47

Authors:

Isabel García García, Kiel Howe, John March-Russell
More details from the publisher
Details from ArXiV

Natural Scherk-Schwarz Theories of the Weak Scale

(2015)

Authors:

Isabel Garcia Garcia, Kiel Howe, John March-Russell
More details from the publisher

Twin Higgs WIMP dark matter

Physical Review D American Physical Society (APS) 92:5 (2015) 055034

Authors:

Isabel García García, Robert Lasenby, John March-Russell
More details from the publisher
Details from ArXiV

Twin Higgs Asymmetric Dark Matter.

Physical review letters 115:12 (2015) 121801

Authors:

Isabel García García, Robert Lasenby, John March-Russell

Abstract:

We study asymmetric dark matter (ADM) in the context of the minimal (fraternal) twin Higgs solution to the little hierarchy problem, with a twin sector with gauged SU(3)^{'}×SU(2)^{'}, a twin Higgs doublet, and only third-generation twin fermions. Naturalness requires the QCD^{'} scale Λ_{QCD}^{'}≃0.5-20  GeV, and that t^{'} is heavy. We focus on the light b^{'} quark regime, m_{b^{'}}≲Λ_{QCD}^{'}, where QCD^{'} is characterized by a single scale Λ_{QCD}^{'} with no light pions. A twin baryon number asymmetry leads to a successful dark matter (DM) candidate: the spin-3/2 twin baryon, Δ^{'}∼b^{'}b^{'}b^{'}, with a dynamically determined mass (∼5Λ_{QCD}^{'}) in the preferred range for the DM-to-baryon ratio Ω_{DM}/Ω_{baryon}≃5. Gauging the U(1)^{'} group leads to twin atoms (Δ^{'}-τ^{'}[over ¯] bound states) that are successful ADM candidates in significant regions of parameter space, sometimes with observable changes to DM halo properties. Direct detection signatures satisfy current bounds, at times modified by dark form factors.
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