Search Strategy for Sleptons and Dark Matter Using the LHC as a Photon Collider
Lydia Beresford
*
and Jesse Liu
†
Department of Physics, University of Oxford, Oxford OX1 3RH, United Kingdom
(Received 3 December 2018; revised manuscript received 22 July 2019; published 3 October 2019)
We propose a search strategy using the LHC as a photon collider to open sensitivity to scalar lepton
(slepton
˜
l) production with masses around 15 to 60 GeV above that of neutralino dark matter
˜
χ
0
1
. This
region is favored by relic abundance and muon ðg − 2Þ
μ
arguments. However, conventional searches are
hindered by the irreduc ible diboson background. We overcome this obstruction by measuring initial state
kinematics and the missing momentum four-vector in proton-tagged ultraperipheral collisions using
forward detectors. We demonstrate sensitivity beyond LEP for slepton masses of up to 200 GeV for
15 ≲ Δmð
˜
l;
˜
χ
0
1
Þ ≲ 60 GeV with 100 fb
−1
of 13 TeV proton collisions. We encourage the LHC
collaborations to open this forward frontier for discovering new physics.
DOI: 10.1103/PhysRevLett.123.141801
Introduction.—Elucidating the elementary properties of
dark matter (DM) is among the most urgent problems in
fundamental physics. The lightest neutralino
˜
χ
0
1
in super-
symmetric (SUSY) extensions of the standard model (SM)
is one of the most motivating DM candidates [1–3].A
favored scenario involves scalar partners of the charged
leptons (sleptons
˜
l) being 1 to tens of GeV above the
˜
χ
0
1
mass. This enables interactions that reduce the
˜
χ
0
1
cosmo-
logical relic abundance to match the observed value [4]
via a mechanism called slepton coannihilation [5,6].
Furthermore, partners of the muon (smuon ˜μ) and neu-
tralinos with masses near the weak scale are a leading
explanation for 3σ to 4σ deviations between measurements
of the muon magnetic moment and SM prediction [7–10].
Remarkably, Large Hadron Collider (LHC) searches for
these key targets have no sensitivity when mass differences
are 15 ≲ Δmð
˜
l;
˜
χ
0
1
Þ ≲ 60 GeV [11–14]. Here, Large
Electron Positron (LEP) collider limits remain the most
stringent, excluding mð
˜
lÞ ≲ 97 GeV [15–17]. Sensitivity
is hindered by an obstruction generic to all LHC search
strategies for invisible DM states and their mediators
[18–32]: the kinematics of colliding quarks and gluons
are immeasurable. Without this initial state information, the
missing momentum four-vector p
miss
left by DM can be
determined only in the plane transverse to the beam (p
miss
T
).
This precludes direct DM mass reconstruction that would
otherwise provide effective discrimination against neutrino
ν backgrounds.
This Letter proposes a search strategy to resolve these
long-standing problems by using the LHC as a photon
collider [33]. In a beam crossing, protons can undergo
an ultraperipheral collision (UPC), where photons from
the electromagnetic fields interact to produce sleptons
exclusively, pp → pðγγ →
˜
l
˜
lÞp. The sleptons decay as
˜
l → l
˜
χ
0
1
, resulting in the very clean final state pð2l þ
p
miss
Þp of our search: two intact protons, two leptons l,
and missing momentum (Fig. 1). As the beam energy is
known, measuring the outgoing proton kinematics deter-
mines the colliding photon momenta and thus p
miss
. This
experimental possibility is opened by the ATLAS Forward
Proton (AFP) [34] and CMS-TOTEM Precision Proton
Spectrometer (CT-PPS) [35,36] forward detectors, which
recorded their first data in 2017 and 2016, respectively.
CMS-TOTEM moreover observed double lepton produc-
tion in high-luminosity proton-tagged events [37], demon-
strating that initial state reconstruction is feasible.
Photon collisions at the LHC reach sufficient rates to
probe rare processes such as SM light-by-light scattering
[38,39], anomalous gauge couplings [40,41], axionlike
particles [42,43], and dark sectors [44,45]. Nonetheless,
FIG. 1. Exclusive pair production of (left panel) scalar leptons
(“sleptons”)
˜
l decaying to dark matter
˜
χ
0
1
and (right panel) SM
diboson WW background using the LHC as a photon collider.
Published by the American Physical Society under the terms of
the Creative Commons Attribution 4.0 International license.
Further distribution of this work must maintain attribution to
the author(s) and the published article’s title, journal citation,
and DOI. Funded by SCOAP
3
.
PHYSICAL REVIEW LETTERS 123, 141801 (2019)
0031-9007=19=123(14)=141801(7) 141801-1 Published by the American Physical Society