# The European Physical Journal C

The European Physical Journal C > 2018 > 78 > 10 > 1-7

The European Physical Journal C > 2018 > 78 > 10 > 1-9

The European Physical Journal C > 2018 > 78 > 10 > 1-8

*CP*violations in $$B^-\rightarrow K^-\pi ^+\pi ^-$$ B-→K-π+π- and $$B^-\rightarrow K^- f_0(500)$$ B-→K-f0(500) decays. We find the experimental data of the localized

*CP*asymmetry in $$B^-\rightarrow K^-\pi ^+\pi ^-$$ B-→K-π+π- decays in the region $$m_{K^-\pi ^+}^2<15$$ mK-π+2<15 $$\mathrm {GeV}^2$$ GeV2 and $$0.08<m_{\pi ^+\pi ^-}^2<0...

The European Physical Journal C > 2018 > 78 > 10 > 1-9

*via*leptogenesis scenario, we consider a reasonable hierarchical structure for Dirac neutrino mass matrix, similar to up-type quark mass matrix. These hypotheses imply a relevant connection between high scale CP violation and low energy one. By requiring a compact heavy neutrino mass spectrum, which allows...

The European Physical Journal C > 2018 > 78 > 10 > 1-10

The European Physical Journal C > 2018 > 78 > 10 > 1-15

The European Physical Journal C > 2018 > 78 > 10 > 1-20

The European Physical Journal C > 2018 > 78 > 10 > 1-11

The European Physical Journal C > 2018 > 78 > 10 > 1-10

*f*(

*R*,

*T*) gravity. To discuss the features of compact stars, we consider that in the interior of the stellar system, the fluid distribution is influenced by MIT bag model equation of state. We construct the field equations by employing Krori–Barua solutions and obtain the...

The European Physical Journal C > 2018 > 78 > 10 > 1-6

The European Physical Journal C > 2018 > 78 > 10 > 1-7

The European Physical Journal C > 2018 > 78 > 10 > 1-9

The European Physical Journal C > 2018 > 78 > 10 > 1-8

The European Physical Journal C > 2018 > 78 > 10 > 1-16

The European Physical Journal C > 2018 > 78 > 10 > 1-20

*Q*is assigned to the right-handed neutrino $$\nu _R$$ νR in order to realise scotogenic Dirac neutrino mass at one-loop level, where three typical value $$Q=-\,\frac{1}{4},-\,4,\frac{3}{2}$$ Q=-14,-4,32...

The European Physical Journal C > 2018 > 78 > 10 > 1-6

The European Physical Journal C > 2018 > 78 > 10 > 1-19

The European Physical Journal C > 2018 > 78 > 10 > 1-11

*Y*(

*R*) to the electromagnetic field invariant $$F^2$$ F2 . After we obtain exact anisotropic solutions to the field equations of the model, we apply the continuity conditions to the solutions at the boundary of the star. Then we find the mass, electric...

The European Physical Journal C > 2018 > 78 > 10 > 1-25

The European Physical Journal C > 2018 > 78 > 10 > 1-6

*W*bosons, $$e^+_{} e^-_{} \rightarrow W^+_{} W^-_{} H$$ e+e-→W+W-H , in the inverse seesaw model. Taking into account all relevant experimental and theoretical constraints, we find sizable effects due to the additional heavy neutrinos up to $$-38\%$$ -38% on the total cross-section...