K. Kovarik
Karlsruhe Institute of Technology
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Featured researches published by K. Kovarik.
Physical Review D | 2009
I. Schienbein; K. Kovarik; J. Morfin; J.F. Owens; F. Olness; C. Keppel; Ji Young Yu
We perform a \chi^2-analysis of Nuclear Parton Distribution Functions (NPDFs) using neutral current charged-lepton Deeply Inelastic Scattering (DIS) and Drell-Yan data for several nuclear targets. The nuclear A dependence of the NPDFs is extracted in a next-to-leading order fit. We compare the nuclear corrections factors F2(Fe)/F2(D) for this charged-lepton data with other results from the literature. In particular, we compare and contrast fits based upon the charged-lepton DIS data with those using neutrino-nucleon DIS data.
Physical Review D | 2015
Julia Harz; B. Herrmann; Michael Klasen; K. Kovarik
We discuss the
Journal of High Energy Physics | 2014
Michael Klasen; C. Klein-Bösing; K. Kovarik; G. Kramer; M. Topp; J.P. Wessels
{\cal O}(\alpha_s)
Physical Review D | 2016
Michael Klasen; K. Kovarik; P. Steppeler
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.
arXiv: High Energy Physics - Phenomenology | 2012
T. Stavreva; Tomas Jezo; K. Kovarik; A. Kusina; F. Olness; J. Yu; I. Schienbein
A bstractNext-to-leading order (NLO) QCD predictions for the production of heavy quarks in proton-proton collisions are presented within three different approaches to quark mass, resummation and fragmentation effects. In particular, new NLO and parton shower simulations with POWHEG are performed in the ALICE kinematic regime at three different centre-of-mass energies, including scale and parton density variations, in order to establish a reliable baseline for future detailed studies of heavy-quark suppression in heavy-ion collisions. Very good agreement of POWHEG is found with FONLL, in particular for centrally produced D0, D+ and D*+ mesons and electrons from charm and bottom quark decays, but also with the generally somewhat higher GM-VFNS predictions within the theoretical uncertainties. The latter are dominated by scale rather than quark mass variations. Parton density uncertainties for charm and bottom quark production are computed here with POWHEG for the first time and shown to be dominant in the forward regime, e.g. for muons coming from heavy-flavour decays. The fragmentation into Ds mesons seems to require further tuning within the NLO Monte Carlo approach.
arXiv: High Energy Physics - Phenomenology | 2013
Julia Harz; Quentin Le Boulc'h; Björn Herrmann; K. Kovarik; Michael Klasen
In this paper, we perform a full next-to-leading order (NLO) QCD calculation of neutralino scattering on protons or neutrons in the MSSM. We match the results of the NLO QCD calculation to the scalar and axial-vector operators in the effective field theory approach. These govern the spin-independent and spin-dependent detection rates, respectively. The calculations have been performed for general bino, wino and higgsino decompositions of neutralino dark matter and required a novel tensor reduction method of loop integrals with vanishing relative velocities and Gram determinants. Numerically, the NLO QCD effects are shown to be of at least of similar size and sometimes larger than the currently estimated nuclear uncertainties. We also demonstrate the interplay of the direct detection rate with the relic density when consistently analyzed with the program
arXiv: High Energy Physics - Phenomenology | 2012
K. Kovarik
\mathtt{DM@NLO}
arXiv: High Energy Physics - Phenomenology | 2018
D. B. Clark; A. Kusina; J. Morfin; Fredrick I. Olness; J.F. Owens; Florian Lyonnet; C. Keppel; J. Yu; T. Ježo; I. Schienbein; E. Godat; K. Kovarik
.
arXiv: High Energy Physics - Phenomenology | 2017
Björn Herrmann; Julia Harz; Michael Klasen; K. Kovarik; P. Steppeler
We analyze the properties of the ACOT scheme for heavy quark production and make use of the MS-Bar massless results at NNLO and N3LO for the structure functions F2 and FL in neutral current deep-inelastic scattering to estimate the higher order corrections. The dominant heavy quark mass effects at higher orders can be taken into account using the massless Wilson coefficients together with an appropriate slow-rescaling prescription implementing the phase space constraints. Combining the exact ACOT scheme at NLO with these expressions should provide a good approximation to the full calculation in the ACOT scheme at NNLO and N3LO.
Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2017) | 2017
Michael Klasen; K. Kovarik; Saskia Schmiemann
We have calculated the full O(as) supersymmetric QCD corrections to neutralino-stop coannihilation into electroweak vector and Higgs bosons within the Minimal Supersymmetric Standard Model (MSSM). We performed a parameter study within the phenomenological MSSM and demonstrated that the studied co-annihilation processes are phenomenologically relevant, especially in the context of a 126 GeV Higgs-like particle. By means of an example scenario we discuss the effect of the full next-to-leading order corrections on the co-annihilation cross section and show their impact on the predicted neutralino relic density. We demonstrate that the impact of these corrections on the cosmologically preferred region of parameter space is larger than the current experimental uncertainty of WMAP data.