Studying Very Light Gravitino at the ILC

TL;DR

This paper explores how to detect and measure very light gravitinos at the ILC, focusing on stau decays and impact parameter distributions to infer gravitino properties and supersymmetry breaking scale.

Contribution

It introduces a method to determine the lifetime and mass of a very light gravitino via impact parameter analysis of stau decays at the ILC.

Findings

Stau lifetime can be measured if longer than ~10^{-14} sec.

The method estimates gravitino mass and SUSY breaking scale.

Effective for stau mass around 100 GeV.

Abstract

A collider signal with a stable gravitino of ${\cal O}(10)$eV mass at the International Linear Collider (ILC) experiment is investigated. Such a light gravitino is generally predicted in the low-scale gauge mediation scenario of the supersymmetry breaking. We particularly focus on the case that the next lightest supersymmetric particle is stau, which eventually decays into a gravitino and a $\tau$-lepton. With such a small gravitino mass, the lifetime of the stau is $10^{-15}$--$10^{-11}$sec, and the produced stau decays before reaching the first layer of the inner detector of the ILC. It is shown, however, that the lifetime can be determined from the distribution of the impact parameter, which is obtained by observing charged tracks caused by decay products of the $\tau$-lepton. This measurement also enables us to estimate the mass of the gravitino and determine the scale of the supersymmetry breaking. Based on a simulation study, we found that the lifetime can be measured when it is longer than $\sim 10^{-14}$sec and the stau mass is about 100GeV.