Casting Light on BSM Physics with SM Standard Candles

TL;DR

This paper demonstrates how measurements of SM Standard Candles, specifically WW cross sections, can be used to set new constraints on electroweak-scale new physics, filling gaps left by previous experiments and addressing anomalies.

Contribution

It introduces a novel approach of using SM Standard Candle measurements to constrain new physics models, particularly light sleptons, complementing existing collider searches.

Findings

WW measurements can constrain light sleptons effectively.

Sleptons can improve the fit to WW data over the SM prediction.

Sleptons can account for the (g-2)_μ anomaly and dark matter relic density.

Abstract

The Standard Model (SM) has had resounding success in describing almost every measurement performed by the ATLAS and CMS experiments. In particular, these experiments have put many beyond the SM models of natural Electroweak Symmetry Breaking into tension with the data. It is therefore remarkable that it is still the LEP experiment, and not the LHC, which often sets the gold standard for understanding the possibility of new color-neutral states at the electroweak (EW) scale. Recently, ATLAS and CMS have started to push beyond LEP in bounding heavy new EW states, but a gap between the exclusions of LEP and the LHC typically remains. In this paper we show that measurements of SM Standard Candles can be repurposed to set entirely complementary constraints on new physics. To demonstrate this, we use WW cross section measurements to set bounds on a set of slepton-based simplified models which fill in the gaps left by LEP and dedicated LHC searches. Having demonstrated the sensitivity of the WW measurement to light sleptons, we also find regions where sleptons can improve the fit of the data compared to the NLO SM WW prediction alone. Remarkably, in those regions the sleptons also provide for the right relic-density of Bino-like Dark Matter and provide an explanation for the longstanding 3 sigma discrepancy in the measurement of (g-2)_\mu.