The contribution of unparticles to the M\(\o\)ller scattering in the Randall-Sundrum model

Van Soa Dang, M. Le, Đào Thị Bích Thủy
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Abstract

The influence of vector, scalar unparticle exchange and photon \((\gamma)\), \(Z\) boson, Higgs-radion \((h,\phi)\) exchange on the fundamental M\(\o\)ller scattering in Randall-Sundrum model is presented. We evaluated the contribution from each exchange in standard model physics and unparticle physics to the final production cross-sections with the apposite energy reach in the current accelerators and colliders. The results indicate that the effect of vector unparticles is larger than its scalar all over the range of collision energy, as much greater than Higgs \((h)\) and radion \((\phi)\) in the low energy. \(Z\) boson exchange also contributes the greatest to the process in both unpolarized and polarized conditions in higher energy regions when compared to photon exchange \((\gamma)\) which normally dominates at the lower energies.
Randall-Sundrum模型中非粒子对M \(\o\) ller散射的贡献
给出了Randall-Sundrum模型中矢量、标量非粒子交换和光子\((\gamma)\)、\(Z\)玻色子、希格斯-辐射\((h,\phi)\)交换对基本M \(\o\) ller散射的影响。我们评估了标准模型物理和非粒子物理中每次交换对当前加速器和对撞机中具有相应能量范围的最终生产截面的贡献。结果表明,在整个碰撞能量范围内,矢量非粒子的效应都大于其标量效应,在低能范围内比希格斯粒子\((h)\)和放射性粒子\((\phi)\)的效应大得多。\(Z\)与光子交换相比,玻色子交换在高能量区域的非极化和极化条件下也对过程贡献最大\((\gamma)\)通常在低能量区域占主导地位。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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