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Collider Implications of Kaluza-Klein Excitations of the Gluons

D. A. Dicus, C. D. McMullen, S. Nandi

Abstract

We consider an asymmetric string compactification scenario in which the SM gauge bosons can propagate into one TeV$^{-1}$-size extra compact dimension. These gauge bosons have associated KK excitations that present additional contributions to the SM processes. We calculate the effects that the KK excitations of the gluons, $g^{\star}$'s, have on multijet final state production in proton-proton collisions at the Large Hadron Collider energy. In the case of dijet final states with very high $p_{{}_T}$, the KK signal due to the exchanges of the $g^{\star}$'s is several factors greater than the SM background for compactification scales as high as about 7 TeV. The high-$p_{{}_T}$ effect is not as dramatic for the direct production of a single on-shell $g^{\star}$, which subsequently decays into $q$-$\bar{q}$ pairs, where the KK signal significantly exceeds the SM three-jet background for compactification scales up to about 3 TeV. We also present our results for the four-jet final state signal from the direct production of two on-shell $g^{\star}$'s.

Collider Implications of Kaluza-Klein Excitations of the Gluons

Abstract

We consider an asymmetric string compactification scenario in which the SM gauge bosons can propagate into one TeV-size extra compact dimension. These gauge bosons have associated KK excitations that present additional contributions to the SM processes. We calculate the effects that the KK excitations of the gluons, 's, have on multijet final state production in proton-proton collisions at the Large Hadron Collider energy. In the case of dijet final states with very high , the KK signal due to the exchanges of the 's is several factors greater than the SM background for compactification scales as high as about 7 TeV. The high- effect is not as dramatic for the direct production of a single on-shell , which subsequently decays into - pairs, where the KK signal significantly exceeds the SM three-jet background for compactification scales up to about 3 TeV. We also present our results for the four-jet final state signal from the direct production of two on-shell 's.

Paper Structure

This paper contains 40 equations, 16 figures.

Figures (16)

  • Figure 1: Relative coupling strengths of vertices involving $g^{\star}$'s. Only the overall factors are shown: The $q$-$\bar{q}$-$g^{\star}$ vertex also involves the SU($3$) matrix element and the Dirac $\gamma_{\mu}$ matrix; triple vertices of $g$'s and $g^{\star}$'s also include the usual SU($3$) structure functions and the momenta factors; and quadruple vertices of $g$'s and $g^{\star}$'s also contain the usual structure function factors as well as the metric tensors $g_{\mu \nu}$. Here, $n$, $m$, and $\ell$ are distinct positive integers ($n \neq m \neq \ell$).
  • Figure 2: Dijet diagrams involving KK excitations of the gluons. The indices $i$ and $j$ represent distinct ($i \neq j$) quark flavors.
  • Figure 3: The contributions of the virtual exchanges of $g^{\star}$'s to the LHC dijet production cross section, $\sigma_{{}_{\mathit{KK}}} = \sigma - \sigma_{{}_{\mathit{SM}}}$, (top) and the ratio of the KK contribution to the SM background, $R = \sigma_{{}_{\mathit{KK}}} / \sigma_{{}_{\mathit{SM}}}$, (bottom) are illustrated as a function of the minimum transverse momentum $p_{{}_T}^{{}^{\mathit{min}}}$ for fixed values of the compactification scale $\mu$. The solid horizontal line represents $\sim 200$ events/yr at the projected integrated luminosity. Discernible bumps in regions for which $p_{{}_T}^{{}^{\mathit{min}}} = k \mu / 2$ are indicated by the corresponding value of $k \in \{1,2,\ldots\}$.
  • Figure 4: Same as Fig. \ref{['fig:gs2a']}, but as a function of the compactification scale $\mu$ for fixed values of the minimum transverse momentum $p_{{}_T}^{{}^{\mathit{min}}}$. The horizontal dashed lines represent the SM background.
  • Figure 5: The partial contributions to the total dijet cross section are shown as a function of $p_{{}_T}^{{}^{\mathit{min}}}$, for $\mu = 3.5$ TeV.
  • ...and 11 more figures