A comment on the impact of CMD-3 e+e−→π+π−e^+e^- \to \pi^+\pi^- cross section measurement on the SM gμ−2g_\mu-2 value

We estimated an impact of the recent CMD-3 measurement of the $e^+e^- \to \pi^+\pi^-$ total cross section at $0.3 < \sqrt{s} < 1.2$ GeV on the leading order hadronic contribution $a_\mu^{had,LO}$ to the muon anomalous magnetic moment $a_\mu = (g_\mu-2)/2$, in presence of comparably precise ISR measurements of the cross section by BaBar and KLOE experiments being in significant tension with the CMD-3. Assuming that all the experiments are affected by yet unidentified systematic effects, to account for the latter, we scaled the experimental uncertainties following the PDG prescription, thus facilitating a consistent joint fit of the world data on the $e^+e^- \to \pi^+\pi^-$ total cross section. The same procedure was applied in all $e^+e^- \to hadrons$ channels contributing to the dispersive estimate of $a_\mu^{had,LO}$. Despite an inclusion of the new CMD-3 $\pi^+\pi^-$ data, our estimate $a_\mu^{had,LO}(e^+e^-) = (696.2 \pm 2.9) \times 10^{-10}$ is consistent with $a_\mu^{had,LO}(e^+e^-)$ values obtained by other authors before publication of the CMD-3 result. Including our $a_\mu^{had,LO}$ value into the SM prediction for $a_\mu$, we obtain $a_\mu^{SM} = (11~659~184 \pm 4_{\mathrm{tot}}) \times 10^{-10}$ which is by $4.7\sigma$ smaller than the world average for the experimental value $a_\mu^{exp} = (11~659~205.9 \pm 2.2) \times 10^{-10}$. We confirm the observation by the CMD-3 authors that their $\sigma(e^+e^- \to \pi^+\pi^-)$ measurement, when taken alone, implies the $a_\mu^{SM}$ prediction consistent with the $a_\mu^{exp}$ at $\sim 1\sigma$ level.Comment: The note contains a comprehensive bibliography on the total e+e- --> hadrons cross section measurements at sqrt(s) < 12 Ge

Black Hole Shadows: How to Fix the Extended Gravity Theory

The first images of black hole shadows open new possibilities to develop modern extended gravity theories. We discuss the shadow calculations in non-rotating case both when $g_{11} = - g_{00}^{-1}$ and $g_{11} \neq - g_{00}^{-1}$. We demonstrate the application to few different models: Horndesky theory with Gauss-Bonnet invariant, loop quantum gravity and conformal gravity. The difference of these theories from shadow models with the theory of general relativity is shown. In addition we show that when the rotation is taken into account the requirements to the observational accuracy decrease