doubly-charged scalars at high-energy and high-precision ... · to be " 0.2 ppb, smaller than...
TRANSCRIPT
Doubly-charged scalars at high-energy andhigh-precision experiments
BHUPAL DEV
Washington University in St. Louis
with M. J. Ramsey-Musolf (UMass) and Y. Zhang (WashU), arXiv:1805.0xxxx
PHENO 2018University of Pittsburgh
May 8, 2018
Outline
Introduction: Energy versus Precision Frontier
Example: LHC versus MOLLER
A case study: Doubly charged scalar
Conclusion
Two Frontiers: Energy versus Precision
[Le Dall, Pospelov, Ritz (PRD ’15)]
Two Frontiers: Energy versus Precision
Complementary and intertwined. Need input from both to probe new physics.
Two Frontiers: Energy versus Precision8
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Example: LHC versus MOLLER
MOLLER Experiment
Measurement Of a Lepton Lepton Electroweak Reaction 8
28 m
liquid hydrogentarget
upstreamtoroid
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detectorsystems
electronbeam
FIG. 7: MOLLER Experiment Overview: Layout of the target, spectrometer and detectors.
Compton-scattered photon or electron measurements.In order to achieve the necessary rate, the liquid hydrogen target is planned to be 150 cm long. This requires a
cryogenic target system capable of handling a heat load of ⇠ 5 kW from the beam. This would be the highest powerliquid hydrogen target constructed, but it would be based on successful experience with the operation of the Qweaktarget which successfully operated up to 180 µA with a total power of 2.9 kW [29]. The final design of the MOLLERtarget will make use of computational fluid dynamics (CFD), a key recent development which has been validated bythe successful operation of the Qweak target. From the physics point of view, the most important design considerationis suppression of density fluctuations at the timescale of the helicity flip rate, which can ruin the statistical reach of theflux integration technique. Preliminary estimates based on operational experience with the Qweak target [29] suggestthat density variation can be maintained at . 26 ppm at 1.92 kHz (compared to the expected counting statisticswidth of ⇠ 83 ppm/pair at 75 µA), corresponding to accepatable 5% excess noise.
A precision collimation system carefully designed to minimize backgrounds will accept all Møller scatteredelectrons in the polar angle range ⇥COM = 60� � 120� (corresponding to a lab polar scattering angle range of 5 mrad< ✓lab < 17 mrad). The spectrometer system that focusses these scattered particles is designed to achieve twogoals: 100% azimuthal acceptance and the ability to focus the scattered Møller flux over a large fractional momentumbite with adequate separation from backgrounds. These considerations have led to a unique solution involving twoback-to-back sets of toroidal coils, one of them of conventional geometry (albeit long and quite skinny) while the otheris of quite novel geometry. Due to the special nature of identical particle scattering, it is possible to achieve 100%azimuthal acceptance in such a system by choosing an odd number of coils. The idea is to accept both forward andbackward (in center of mass angle) Møllers in each � bite. Since these are identical particles, those that are accepted inone � bite also represent all the statistics available in the � bite that is diametrically opposed (180� +�), which is thesector that is blocked due to the presence of a toroidal coil. An event with a forward angle scattered Møller electronthat azimuthally scatters into a blocked sector is detected via its backward angle scattered partner in the open sectordiametrically opposed, and vice versa. The focussing and separation of the scattered Møller electrons is challengingdue to their large scattered energy range E0
lab = 1.7 � 8.5 GeV and the need to separate them from the primarybackground of elastic and inelastic electron-proton scattering. The solution is a combination of two toroidal magnetswhich together act in a non-linear way on the charged particle trajectories. The first is a conventional toroid placed 6m downstream of the target and the second, a novel “hybrid” toroid placed between 10 and 16 m downstream of thetarget. Each of the two toroidal fields is constructed out of seven identical coils uniformly spaced in the azimuth. The“hybrid” toroid has several novel features to provide the required field to focus the large range of electron scatteringangles and momenta. It has four current return paths, as shown in Fig. 8 and some novel bends that minimize thefield in certain critical regions. A preliminary engineering design of this hybrid toroid with realistic conductor, water
Scattering of longitudinally polarized electrons off unpolarized electrons.Upgraded 11 GeV electron beam in Hall A at JLab.
Parity-Violating Asymmetry
APV =σR − σL
σR + σL
3
electroweak theory prediction at tree level in terms of the weak mixing angle is QeW = 1�4 sin2 ✓W ; this is modified at
the 1-loop level [4–6] and becomes dependent on the energy scale at which the measurement is carried out, i.e. sin2 ✓W
“runs”. It increases by approximately 3% compared to its value at the scale of the Z0 boson mass, MZ ; this and otherradiative corrections reduce Qe
W to 0.0435, a ⇠ 42% change of its tree level value of ⇠ 0.075 (when evaluated at MZ).The dominant e↵ect comes from the “� � Z mixing” diagrams depicted in Fig. 2 [5]. The prediction for APV for theproposed experimental design is ⇡ 33 parts per billion (ppb) and the goal is to measure this quantity with an overallprecision of 0.7 ppb and thus achieve a 2.4% measurement of Qe
W . The reduction in the numerical value of QeW due
to radiative corrections leads to increased fractional accuracy in the determination of the weak mixing angle, ⇠ 0.1%,matching the precision of the single best such determination from measurements of asymmetries in Z0 decays in thee+e� colliders LEP and SLC. An important point to note is that, at the proposed level of measurement accuracy ofAPV , the Standard Model (SM) prediction must be carried out with full treatment of one-loop radiative correctionsand leading two-loop corrections. The current error associated with radiative corrections for MOLLER is estimatedto be ⇠ 0.2 ppb, smaller than the expected 0.7 ppb overall precision. There is an ongoing e↵ort to investigate severalclasses of diagrams beyond one-loop [31–33], and a plan has been formulated to evaluate the complete set of two-loopcorrections at MOLLER kinematics by 2016; such corrections are estimated to be already smaller than the MOLLERstatistical error. The existing work makes it clear that the theoretical uncertainties for the purely leptonic Møller PVare well under control, and the planned future work will reinforce that conclusion.
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FIG. 1: Feynman diagrams for Møller scattering at tree level (reproduced from Ref. [5])
Z
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FIG. 2: Significant 1-loop radiative corrections: � � Z mixing diagrams and W -loop contribution to the anapole moment(reproduced from Ref. [5])
The proposed MOLLER measurement will make a precision (2.4% relative) measurement of a suppressed StandardModel observable (Qe
W ⇠ 0.0435) resulting in sensitivity to new neutral current amplitudes as weak as ⇠ 10�3 · GF
from as yet undiscovered dynamics beyond the Standard Model. The fact that the proposed measurement providessuch a sensitive probe of TeV-scale dynamics beyond the SM (BSM) is a consequence of a very precise experimentalgoal (⇠ 10�3 · GF ), the energy scale of the reaction (Q2 ⌧ M2
Z), and the ability within the electroweak theory toprovide quantitative predictions with negligible theoretical uncertainty. The proposed measurement is likely the onlypractical way, using a purely leptonic scattering amplitude at Q2 ⌧ M2
Z , to make discoveries in important regions ofBSM space in the foreseeable future at any existing or planned facility worldwide.
The weak mixing angle sin2 ✓W has played a central role in the development and validation of the electroweaktheory, especially testing it at the quantum loop level, which has been the central focus of precision electroweakphysics over the past couple of decades. To develop the framework, one starts with three fundamental experimentalinputs characterizing, respectively, the strength of electroweak interactions, the scale of the weak interactions, and thelevel of photon-Z0 boson mixing. The three fundamental inputs are chosen to be ↵ (from the Rydberg constant), GF
(from the muon lifetime) and MZ (from the LEP Z0 line-shape). Precise theoretical predictions for other experimentalobservables at the quantum-loop level can be made if experimental constraints on the strong coupling constant andheavy particle masses, such as mH and the top quark mass, mt, are also included.
Precision measurements of the derived parameters such as the W boson mass MW , and the weak mixing anglesin2 ✓W are then used to test the theory at the level of electroweak radiative corrections. Consistency (or lack thereof)of various precision measurements can then be used to search for indications of BSM physics. One important new
ASMPV = mE
GF√2πα
2y(1− y)
1 + y4 + (1− y)4 QeW
For the MOLLER design, ASMPV ≈ 33 ppb (including 1-loop effect).
Goal: δAPV = 0.7 ppb. [J. Benesch et al. [MOLLER Collaboration], arXiv:1411.4088 [nucl-ex]]
Achieve a 2.4% precision in the measurement of QeW .
Sensitive to New Physics
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Λ√|g2
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2GF|∆QeW |' 7.5 TeV
Case Study: Doubly Charged Scalar
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MPV ∼|(fL)ee|2
2(M±±L )2(eLγ
µeL)(eLγµeL) + (L↔ R) .
MOLLER Sensitivity :MH±±
L,R
|(fL,R)ee|& 5.3 TeV .
Case Study: Doubly Charged Scalar
100 1000 10410-3
10-2
0.1
1
10
MHL±± [GeV]
δAPV[ppb
]
MOLLER prospect|(fL )ee |
=1
|(fL )ee |=0.1
|(fL )ee |=0.01
[BD, Ramsey-Musolf, Zhang ’18]
Why Doubly Charged Scalar?
Neutrino Mass via Type-II Seesaw
LY = − (fL)ij ψTL, iCiσ2∆LψL, j + H.c.
mν =√
2 fLv∆ = UmνUT .
[Schechter, Valle (PRD ’80); Mohapatra, Senjanovic (PRD ’81); Lazarides, Shafi, Wetterich (NPB ’81)]
Fixes the elements of fL (up to an overall scale)
LFV Constraints
ProcessExperimental limit
on BRConstraint on Bound ×
(MHL
100 GeV
)2
µ→ eγ < 4.2× 10−13 |(f †L fL)eµ| < 2.4× 10−6
µ→ 3e < 1.0× 10−12 |(fL)µe||(fL)ee| < 2.3× 10−7
τ → eγ < 3.3× 10−8 |(f †L fL)eτ | < 1.6× 10−3
τ → µγ < 4.4× 10−8 |(f †L fL)µτ | < 1.9× 10−3
τ → e+e−e− < 2.7× 10−8 |(fL)τe||(fL)ee| < 9.2× 10−5
τ → µ+µ−e− < 2.7× 10−8 |(fL)τµ||(fL)µe| < 6.5× 10−5
τ → e+µ−µ− < 1.7× 10−8 |(fL)τe||(fL)µµ| < 7.3× 10−5
τ → e+e−µ− < 1.8× 10−8 |(fL)τe||(fL)µe| < 5.3× 10−5
τ → µ+e−e− < 1.5× 10−8 |(fL)τµ||(fL)ee| < 6.9× 10−5
τ → µ+µ−µ− < 2.1× 10−8 |(fL)τµ||(fL)µµ| < 8.1× 10−5
[BD, Rodejohann, Vila (NPB ’17)]
MOLLER versus LFV
10-2 0.1 1 1010-3
10-2
0.1
1
10
vΔ [eV]
|(f L) ee|
NH, MHL±± = 1 TeV
excluded by μ→eee
excluded by μ→eγ
MOLLER prospect
[BD, Ramsey-Musolf, Zhang ’18]
MOLLER versus LFV
10-2 0.1 1 10
10-2
0.1
1
10
vΔ [eV]
|(f L) ee|
IH, MHL±± = 1 TeV
excluded byμ→eee
excluded byμ→eγ
MOLLERprospect
[BD, Ramsey-Musolf, Zhang ’18]
Parity-Violating Left-Right Model
LY ⊃ − (fR)ij ψTR, iCiσ2∆RψR, j + H.c..
Could have fR 6= fL at low scale. [Chang, Mohapatra, Parida (PRL ’84)]
fR is not related to the neutrino oscillation data.
LFV constraints do not restrict (fR)ee anymore.Other relevant constraints:
Neutrinoless double beta decayBhabha scattering at LEP: e+e− → e+e−.Drell-Yan process at LHC: pp → γ∗/Z∗ → H++H−−.
Future prospects at ILC/CLIC: e+e− → e±e±H∓∓R and e±γ → e∓H±±R .[BD, Mohapatra, Zhang ’18]
Parity-Violating Left-Right Model
0.5 1 5 10
10-3
10-2
0.1
1
10
MHR
±± [TeV]
|(f R) ee|
parity-violating case
ee→ee
MOLLER
dileptonlimits
0νββ [NH
]
[IH]
ILCCLIC
perturbative limit
[BD, Ramsey-Musolf, Zhang ’18]
Conclusion
Complementarity between the high-energy and high-precisionexperiments.
We considered a case study of doubly-charged scalars.
Can be probed at the MOLLER experiment up to ∼ 20 TeV.
For the parity-violating left-right scenario, goes well beyond the currentconstraints, as well as the future collider sensitivities.