Standard model calculations for precision observables beyond one loop

1998 ◽  
Vol 66 (1-3) ◽  
pp. 63-66
Author(s):  
B. Krause
1991 ◽  
Vol 143 ◽  
pp. 81-86
Author(s):  
W.-R. Hamann

Wolf-Rayet stars represent an important stage in the evolution of massive stars, but are only poorly understood so far. For a better knowledge one might determine their effective temperatures, luminosities and atmospheric compositions. But the emission-line dominated Wolf-Rayet spectra were not accessible to a quantitative analysis for a long time, because “standard” model calculations for static, plane-parallel stellar atmospheres are not adequate to that type of stars.


1990 ◽  
Vol 237 (2) ◽  
pp. 252-255 ◽  
Author(s):  
Robert Grigjanis ◽  
Patrick J. O'Donnell ◽  
Mark Sutherland ◽  
Henri Navelet

1992 ◽  
Vol 07 (36) ◽  
pp. 3357-3364 ◽  
Author(s):  
TOSHIO NUMAO

The status of experimental tests of electron-muon universality in weak interactions is reviewed. The average of the new measurements of the π+→e+ν branching ratio, R ave =Γ(π→eν+π→eνγ)/Γ(π→μν+π→μνγ)=(1.2312±0.0037)×10−4, is consistent with standard model calculations R th =(1.234±0.001)×10−4 and confirms the hypothesis of electron-muon universality at the 0.2% level.


2021 ◽  
Vol 136 (9) ◽  
Author(s):  
S. Heinemeyer ◽  
S. Jadach ◽  
J. Reuter

AbstractHigh-precision experimental measurements of the properties of the Higgs boson at $$\sim 125$$ ∼ 125  GeV as well as electroweak precision observables such as the W-boson mass or the effective weak leptonic mixing angle are expected at future $$e^+e^-$$ e + e - colliders such as the FCC-ee. This high anticipated precision has to be matched with theory predictions for the measured quantities at the same level of accuracy. We briefly summarize the status of these predictions within the standard model and of the tools that are used for their determination. We outline how the theory predictions will have to be improved in order to reach the required accuracy, and also comment on the simulation frameworks for the Higgs and EW precision program.


2021 ◽  
Vol 81 (8) ◽  
Author(s):  
B. C. Allanach ◽  
J. Eliel Camargo-Molina ◽  
Joe Davighi

AbstractWhile it is known that third family hypercharge models can explain the neutral current B-anomalies, it was hitherto unclear whether the $$Z-Z^\prime $$ Z - Z ′ mixing predicted by such models could simultaneously fit electroweak precision observables. Here, we perform global fits of several third family hypercharge models to a combination of electroweak data and those data pertinent to the neutral current B-anomalies. While the Standard Model is in tension with this combined data set with a p-value of .0007, simple versions of the models (fitting two additional parameters each) provide much improved fits. The original Third Family Hypercharge Model, for example, has a p-value of $${.065}$$ . 065 , with $$\sqrt{\Delta \chi ^2}=6.5\sigma $$ Δ χ 2 = 6.5 σ .


2005 ◽  
Vol 20 (29) ◽  
pp. 2199-2214
Author(s):  
THOMAS ZIEGLER

By reviewing the status of time-dependent CP-violation in b →s transitions and double charmonium production in e+e- collisions, two examples of the rich and exciting physics outcome from the B-factories are presented. Both analyses exhibited significant differences in measurement and standard model calculations in the last two years and therefore received particular interest. After a short introduction into the subjects, the results from BaBar and Belle are presented and discussed.


1994 ◽  
Vol 09 (12) ◽  
pp. 1105-1120 ◽  
Author(s):  
DIRK KREIMER

We give a new method for the reduction of tensor integrals to finite integral representations and uv divergent analytic expressions. This includes a new method for the handling of the γ-algebra.


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