Julia Harz
University College London
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Featured researches published by Julia Harz.
Physical Review Letters | 2014
Frank F. Deppisch; Julia Harz; Martin Hirsch
Measuring a nonzero value for the cross section of any lepton number violating (LNV) process would put a strong lower limit on the washout factor for the effective lepton number density in the early Universe at times close to the electroweak phase transition and thus would lead to important constraints on any high-scale model for the generation of the observed baryon asymmetry based on LNV. In particular, for leptogenesis (LG) models with masses of the right-handed neutrinos heavier than the mass scale observed at the LHC, the implied large washout factors would lead to a violation of the out-of-equilibrium condition and exponentially suppress the net lepton number produced in such LG models. We thus demonstrate that the observation of LNV processes at the LHC results in the falsification of high-scale LG models. However, no conclusions about the viability of LG models can be drawn from the nonobservation of LNV processes.
Physical Review D | 2015
Frank F. Deppisch; Julia Harz; Wei-Chih Huang; Martin S. Hirsch; Heinrich Päs
Interactions that manifest themselves as lepton number violating processes at low energies in combination with sphaleron transitions typically erase any preexisting baryon asymmetry of the Universe. In this article, we discuss the constraints obtained from an observation of neutrinoless double beta decay in this context. If a new physics mechanism of neutrinoless double beta decay other than the standard light neutrino exchange is observed, typical scenarios of high-scale baryogenesis will be excluded unless the baryon asymmetry is stabilized via some new mechanism. We also sketch how this conclusion can be extended beyond the first lepton generation by incorporating lepton flavor violating processes.
Physical Review D | 2015
Julia Harz; B. Herrmann; Michael Klasen; K. Kovarik
We discuss the
Physical Review D | 2015
Julia Harz; B. Herrmann; Michael Klasen; K. Kovařík; M. Meinecke
{\cal O}(\alpha_s)
Journal of Cosmology and Astroparticle Physics | 2015
John Ellis; Tomás E. Gonzalo; Julia Harz; Wei Chih Huang
supersymmetric QCD corrections to neutralino-stop coannihilation into a top quark and a gluon in the Minimal Supersymmetric Standard Model (MSSM). This particular channel can be numerically important in wide ranges of the MSSM parameter space with rather light stops. We discuss technical details such as the renormalization scheme and the phase-space slicing method with two cutoffs. We also comment on improvements with respect to earlier works on the given process. Further, we study for the first time the phenomenologically very interesting interplay of neutralino-stop coannihilation with neutralino-pair annihilation into quark pairs taking the full next-to-leading order SUSY-QCD corrections into account. We demonstrate that the numerical impact of these corrections on the total (co)annihilation cross section and finally on the theoretically predicted neutralino relic density is significant.
International Journal of Modern Physics A | 2015
Julia Harz; Wei-Chih Huang; Heinrich Päs
We present the full
Physical Review D | 2018
Julia Harz; Kalliopi Petraki
\mathcal{O}(\alpha_s)
Physical Review D | 2018
Frank F. Deppisch; Lukas Graf; Julia Harz; Wei-Chih Huang
supersymmetric QCD corrections for stop-anti-stop annihilation into electroweak final states within the Minimal Supersymmetric Standard Model (MSSM). We also incorporate Coulomb corrections due to gluon exchange between the incoming stops. Numerical results for the annihilation cross sections and the predicted neutralino relic density are presented. We show that the impact of the radiative corrections on the cosmologically preferred region of the parameter space can become larger than the current experimental uncertainty, shifting the relic bands within the considered regions of the parameter space by up to a few tens of GeV.
Nuclear and Particle Physics Proceedings | 2016
Julia Harz; B. Herrmann; Michael Klasen; K. Kovarik; M. Meinecke; P. Steppeler
We analyse the prospects for constructing hybrid models of inflation that provide a dynamical realisation of the apparent closeness between the supersymmetric GUT scale and the possible scale of cosmological inflation. In the first place, we consider models based on the flipped SU(5)
arXiv: High Energy Physics - Phenomenology | 2014
Frank F. Deppisch; Julia Harz
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