C. Konig
3 Papers
C. Konig is an academic researcher. The author has contributed to research in topics: Star formation & Protostar. The author has co-authored 2 publications.
Chat about Author
Papers
Stringent test of QED with hydrogenlike tin
Jonathan Morgner,Bingsheng Tu,C. Konig,Fabian Heiße,H. Bekker,B. Sikora,Chunhai Lyu,Vladimir A. Yerokhin,Zoltán Harman,J. R. Crespo López-Urrutia,Christoph H. Keitel,Sven Sturm,K. I. F. Physics,69117 Heidelberg,German,Helmholtz-Institut,Gsi Helmholtzzentrum fur Schwerionenforschung,Mainz 55128 +17 more
- 13 Jul 2023
Abstract: Inner-shell electrons naturally sense the electric field close to the nucleus, which can reach extreme values beyond $10^{15}\,\text{V}/\text{cm}$ for the innermost electrons. Especially in few-electron highly charged ions, the interaction with the electromagnetic fields can be accurately calculated within quantum electrodynamics (QED), rendering these ions good candidates to test the validity of QED in strong fields. Consequently, their Lamb shifts were intensively studied in the last decades. Another approach is the measurement of $g$ factors in highly charged ions. However, so far, either experimental accuracy or small field strength in low-$Z$ ions limited the stringency of these QED tests. Here, we report on our high-precision, high-field test of QED in hydrogenlike $^{118}$Sn$^{49+}$. The highly charged ions were produced with the Heidelberg-EBIT (electron beam ion trap) and injected into the ALPHATRAP Penning-trap setup, where the bound-electron $g$ factor was measured with a precision of 0.5 parts-per-billion. For comparison, we present state-of-the-art theory calculations, which together test the underlying QED to about $0.012\,\%$, yielding a stringent test in the strong-field regime. With this measurement, we challenge the best tests via the Lamb shift and, with anticipated advances in the $g$-factor theory, surpass them by more than an order of magnitude.
OGHReS: Star formation in the Outer Galaxy (ℓ = 250○-280○)
James Urquhart,C. Konig,D. Colombo,A. Karska,Friedrich Wyrowski,Karl M. Menten,T. Moore,J. Brand,D. Elia,Andrea Giannetti,Silvia Leurini,M. Figueira,M.-Y. Lee,M. D. U. O. Kent,Mpifr,Universityof Bonn,N. C. University,Liverpool John Moores University,Inaf-Bologna,INAF-Roma,INAF-Selargius,National Centre for Nuclear Research Warazawa,Korea Astronomy,S. S. Institute,U. Chile +24 more
TL;DR: OGHReS provides refined velocities, distances, and physical properties for a large sample of clumps in the outer Galaxy. The data reveal a decreasing luminosity-to-mass ratio and similar surface density for protostellar clumps across the Galactic disc.
2
Far-infrared line emission from the outer Galaxy cluster Gy 3-7 with SOFIA/FIFI-LS: Physical conditions and UV fields
Ngan M. Le,Agata Karska,M. Figueroa,Marta Sewilo,Artur Mirocha,J. Fischer,Maja Ka'zmierczak-Barthel,Ralf Klein,M. Gawro'nski,M. P. Koprowski,Klaudia Kowalczyk,William J. Fischer,Karl M. Menten,Friedrich Wyrowski,C. Konig,Lars E. Kristensen +15 more
- 17 Apr 2023
TL;DR: In this paper , the authors quantify the FIR line emission and determine the spatial distribution of the CO rotational temperature, ultraviolet (UV) radiation field, and H2 number density toward the embedded cluster Gy 3-7 in the CMa-l224 star-forming region, whose metallicity is expected to be intermediate between that of the LMC and the Solar neighborhood.