Zobrazeno 1 - 10
of 5 588
pro vyhledávání: '"Ward, B."'
Autor:
Huang, Zhenguang, Toth, Gabor, Huang, Jia, Sachdeva, Nishtha, van der Holst, Bart, Manchester, Ward B.
A potential field solution is widely used to extrapolate the coronal magnetic field above the Sun's surface to a certain height. This model applies the current-free approximation and assumes that the magnetic field is entirely radial beyond the sourc
Externí odkaz:
http://arxiv.org/abs/2403.01712
Variations in the dust emissivity index, $\beta$, within and between galaxies, are evidence that the chemistry and physics of dust must vary on large scales, although the nature of the physical and/or chemical variations is still unknown. In this pap
Externí odkaz:
http://arxiv.org/abs/2402.05182
There is a continuing effort to support and prepare the precision physics programs for the present and planned future colliders such as HL-LHC, FCC, CLIC, CEPC, and CPPC. We discuss new results from IR-improved amplitude-based resummation in quantum
Externí odkaz:
http://arxiv.org/abs/2310.09962
We extend the YFS IR resummation theory to include all of the attendant collinear contributions which exponentiate. This improves the original YFS formulation in which only a part of these contributions was exponentiated. We show that the new resumme
Externí odkaz:
http://arxiv.org/abs/2303.14260
Autor:
Hagimoto, M., Bakx, T. J. L. C., Serjeant, S., Bendo, G. J., Urquhart, S. A., Eales, S., Harrington, K. C., Tamura, Y., Umehata, H., Berta, S., Cooray, A. R., Cox, P., De Zotti, G., Lehnert, M. D., Riechers, D. A., Scott, D., Temi, P., van der Werf, P. P., Yang, C., Amvrosiadis, A., Andreani, P. M., Baker, A. J., Beelen, A., Borsato, E., Buat, V., Butler, K. M., Dannerbauer, H., Dunne, L., Dye, S., Enia, A. F. M., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Ivison, R. J., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Neri, R., Omont, A., Perez-Fournon, I., Sedgwick, C., Smith, M. W. L., Stanley, F., Verma, A., Vlahakis, C., Ward, B., Weiner, C., Weiss, A., Young, A. J.
We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies between redshifts 1.4 to 4.6 detected by the Atacama Large Millimetre/submillimetre Array. These lines include a total of 156 CO, [C I], and H2O emission lines
Externí odkaz:
http://arxiv.org/abs/2303.04830
Autor:
Sachdeva, Nishtha, Manchester, Ward B, Sokolov, Igor, Huang, Zhenguang, Pevtsov, Alexander, Bertello, Luca, Pevtsov, Alexei A., Toth, Gabor, van der Holst, Bart
We explore model performance for the Alfven Wave Solar atmosphere Model (AWSoM) with near-real-time (NRT) synoptic maps of the photospheric vector magnetic field. These maps, produced by assimilating data from the Helioseismic Magnetic Imager (HMI) o
Externí odkaz:
http://arxiv.org/abs/2212.05138
Autor:
Aktukmak, Mehmet, Sun, Zeyu, Bobra, Monica, Gombosi, Tamas, Manchester, Ward B., Chen, Yang, Hero, Alfred
In this paper, we consider incorporating data associated with the sun's north and south polar field strengths to improve solar flare prediction performance using machine learning models. When used to supplement local data from active regions on the p
Externí odkaz:
http://arxiv.org/abs/2212.01730
Publikováno v:
PoS(ICHEP2022)887
KKMChh adapts the CEEX (Coherent Exclusive Exponentiation) formalism of the Monte Carlo Program KKMC for Z boson production and decay to hadron scattering. Amplitude-level soft photon exponentiation of initial and final state radiation, together with
Externí odkaz:
http://arxiv.org/abs/2211.17177
Publikováno v:
PoS(ICHEP2022)1204
We present an overview of the use of IR-improvement of unintegrable singularities in the infrared regime via amplitude-based resummation in $\mathrm{QED} \times \mathrm{QCD}$ $\subset$ $\mathrm{SU}(2)_L \times \mathrm{U}_1 \times \mathrm{SU}(3)^c$. W
Externí odkaz:
http://arxiv.org/abs/2211.14904
Publikováno v:
PoS(ICHEP2022)1214
For both the FCC-ee and the ILC, to exploit properly the respective precision physics program, the theoretical precision tag on the respective luminosity will need to be improved from the analogs of the $ 0.054 \% (0.061\%)$ results at LEP at $M_Z$,
Externí odkaz:
http://arxiv.org/abs/2211.14230