Decoding the nature of Dark Matter at current and future experiments - - PowerPoint PPT Presentation

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Decoding the nature of Dark Matter at current and future experiments - - PowerPoint PPT Presentation

Decoding the nature of Dark Matter at current and future experiments Alexander Belyaev Southampton University & Rutherford Appleton Laboratory June 10 , 2020, Particle Physics Seminar Alexander Belyaev Decoding the nature of DM 1 Why


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Alexander Belyaev 1 Decoding the nature of DM

Alexander Belyaev

Southampton University & Rutherford Appleton Laboratory

Decoding the nature of Dark Matter

at current and future experiments

June 10 , 2020, Particle Physics Seminar

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Alexander Belyaev 2 Decoding the nature of DM

Why Dark Matter (DM) is in the main focus after Higgs discovery?

statistics of publications based on inSPIRE database

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Alexander Belyaev 3 Decoding the nature of DM

Because while Higgs Discovery has finished the SM puzzle...

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Alexander Belyaev 4 Decoding the nature of DM

Fine-tuning problem Dark Matter problem The origin of matter/anti-matter asymmetry Connection to GUT & couplings unification The Nature of Higgs Boson

… it became obvious that the SM itself is the piece of some (more) complete and consistent BSM theory

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Alexander Belyaev 5 Decoding the nature of DM

Fine-tuning problem Dark Matter problem The origin of matter/anti-matter asymmetry Connection to GUT & couplings unification The Nature of Higgs Boson

… it became obvious that the SM itself is the piece of some (more) complete and consistent BSM theory

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Alexander Belyaev 6 Decoding the nature of DM

CMB: WMAP and PLANCK Large Scale Structures Gravitational lensing Bullet cluster Galactic rotation curves

DM is strong and very appealing evidence for BSM!

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Alexander Belyaev 7 Decoding the nature of DM

DM is very appealing even though we know almost nothing about it!

Spin ? symmetry behind stability V No

Couplings

Weak Higgs Quarks/gluons Leptons New mediators gravity

Stable

Yes Thermal relic Mass No Yes ? ? ? ? ? ? ? ? ? ? ? ?

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Alexander Belyaev 8 Decoding the nature of DM

How we can decode the fundamental nature of Dark Matter?

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Alexander Belyaev 9 Decoding the nature of DM

How we can decode the fundamental nature of Dark Matter? We need a DM signal first!

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Alexander Belyaev 10 Decoding the nature of DM

How we can decode the fundamental nature of Dark Matter? We need a DM signal first! But at the moment we can:

➱ understand what kind of DM is already

excluded

➱ explore theory space and prepare ourselves to

discovery and decoding of DM

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Alexander Belyaev 11 Decoding the nature of DM

Collaborators & Projects

I.Ginzburg, D.Locke, A. Freegard, T. Hosken, AB arXiv:2006.xxxxx S.Prestel, F.Rojas-Abate,J.Zurita, AB arXiv:2006.xxxxx S.Novaes, P.Mercadante, C.S. Moon,T.Tomei,

  • S. Moretti, M.Tomas, L. Panizzi, AB

arXiv:1809.00933 G.Cacciapaglia, J.McKay, D. Marin, A.Zerwekh, AB arXiv:1808.10464 E.Bertuzzo, C.Caniu, G. di Cortona, O.Eboli,

  • F. Iocco, A.Pukhov, AB

arXiv:1807.03817

  • T. Flacke, B. Jain, P. Schaefers, AB

arXiv:1707.07000

  • G. Cacciapaglia, I. Ivanov, F. Rojas, M. Thomas, AB

arXiv:1612.00511

  • I. Shapiro, M. Thomas, AB

arXiv:1611.03651

  • L. Panizzi, A. Pukhov, M.Thomas, AB

arXiv:1610.07545

  • D. Barducci, A.Bharucha, W. Porod, V. Sanz, AB

arXiv:1504.02472

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Alexander Belyaev 12 Decoding the nature of DM

DM candidates: interaction vs mass

http://science.energy.gov/hep/hepap/reports/

Planck mass BH remnants: tiny black holes protected by gravity effects [Chen '04] from decay via Hawking radiation Wimpzillas: very massive non-thermal WIMPs [Kolb,Chung,Riotto'98] Q-balls: topological solitons that occur in QFT [Coleman '86] EW scale WIMPs, protected by parity – LSP, LKP, LTP particles SuperWIMPs: electrically and color neutral DM interacting with much smaller strength (perhaps

  • nly gravitationally)

Neutrinos: usual neutrinos are too light- HDM, subdominant component

  • nly (to be consistent with large scale

structures); but heavier gauge singlet neutrinos can be CDM Axions: is replaced by a quantum field, the potential energy allows the field to relax to near zero strength, axion as a consequence

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Alexander Belyaev 13 Decoding the nature of DM

DM candidates: interaction vs mass

http://science.energy.gov/hep/hepap/reports/

Planck mass BH remnants: tiny black holes protected by gravity effects [Chen '04] from decay via Hawking radiation Wimpzillas: very massive non-thermal WIMPs [Kolb,Chung,Riotto'98] Q-balls: topological solitons that occur in QFT [Coleman '86] EW scale WIMPs, protected by parity – LSP, LKP, LTP particles SuperWIMPs: electrically and color neutral DM interacting with much smaller strength (perhaps

  • nly gravitationally)

Neutrinos: usual neutrinos are too light- HDM, subdominant component

  • nly (to be consistent with large scale

structures); but heavier gauge singlet neutrinos can be CDM Axions: is replaced by a quantum field, the potential energy allows the field to relax to near zero strength, axion as a consequence

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Alexander Belyaev 14 Decoding the nature of DM

Mass range for thermal DM

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Alexander Belyaev 15 Decoding the nature of DM

T.Tait

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Alexander Belyaev 16 Decoding the nature of DM

Minimal Consistent models

universal building block for full models

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Alexander Belyaev 17 Decoding the nature of DM

Correct Relic density: efficient (co) annihilation at the time

  • f early Universe

Dark Matter (DM) Signatures

Efficient annihilation now: Indirect Detection Efficient scattering off nuclei: Direct Detection Efficient production at colliders

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Alexander Belyaev 18 Decoding the nature of DM

Efficient annihilation now: Indirect (ID) DM Detection Efficient scattering off nuclei: DM Direct Detection (DD)

Efficient production at colliders

Complementarity of DM searches

Important: there is no 100%correlation between signatures above. E.g. the high rate of annihilation does not always guarantee high rate for DD! Actually there is a great complementarity in this:

  • In case of NO DM Signal – we can efficiently exclude DM models
  • In case of DM signal – we have a way to determine the nature of DM

Example of DM interactions with negligible/suppressed DD rates

DM DM DM DM W/Z W/Z W/Z W/Z

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Alexander Belyaev 19 Decoding the nature of DM

Direct Dark Matter Detection

Search for the recoil energy of a nucleus in an underground detector after collision with a WIMP Elastic recoil energy Minimum WIMP speed required to produce a recoil energy -

limitation in low DM mass region!

The differential event rate (per unit detector mass):

the source of uncertainty from the halo integral – from DM velocity and density distributions

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Alexander Belyaev 20 Decoding the nature of DM

Latest XENON 1T results

The limit scales linearly with MDM 10-46 cm2 = 10-10 pb

arXiv:1805.12562

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Alexander Belyaev 21 Decoding the nature of DM

Power of DM DD to rule out theory space

ArXiv:1310.8327 Snowmass CF1 Summary

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Alexander Belyaev 22 Decoding the nature of DM

Power of DM DD to rule out theory space

Inert 2 Higgs Doublet Model

scalar DM

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Alexander Belyaev 23 Decoding the nature of DM

Power of DM DD to rule out theory space

Inert 2 Higgs Doublet Model

scalar DM

Cacciapaglia, Ivanov, Rojas, Thomas, AB arXiv:1610.07545 Novaes, Mercadante, Moon,Tomei, Moretti,Tomas, Panizzi, AB arXiv:1809.00933

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Alexander Belyaev 24 Decoding the nature of DM

Power of DM DD to rule out theory space

Vector DM (VDM) Model

DM from vector triplet SM gauge coupling VDMVDMH coupling is the

  • nly free parameter

a H H V V Z V- V+

AB,Cacciapaglia, McKay, Martin, Zerwekh, arXiv:1808.10464

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Alexander Belyaev 25 Decoding the nature of DM

The probe of VDM parameter space

The relic density map in MV- a parameter space

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Alexander Belyaev 26 Decoding the nature of DM

The probe of VDM parameter space

DM DD constraints from XENON1T The relic density map in MV- a parameter space

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Alexander Belyaev 27 Decoding the nature of DM

The probe of VDM parameter space

+relic density constraints from PLANCK: an upper limit on DM mass

ZENON 1T + Planck excludes both large HVDMVDM couplings and large MDM The lower masses (rest of space) can be covered at colliders DM DD constraints from XENON1T The relic density map in MV- a parameter space

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Alexander Belyaev 28 Decoding the nature of DM

The probe of VDM parameter space

DM DD constraints from XENON1T

+Higgs data +lower limit on relic density +relic density constraints from PLANCK: an upper limit on DM mass

The relic density map in MV- a parameter space

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Alexander Belyaev 29 Decoding the nature of DM

DM DD interplay with Collider Searches

process DM DM q q

?

detector

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Alexander Belyaev 30 Decoding the nature of DM

Nothing! DM DM q q q process detector

Hunting for DM at Colliders

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Alexander Belyaev 31 Decoding the nature of DM

Hunting for DM at Colliders

High PT jet Large missing PT (2DM)

DM DM q q g

monojet signature

process detector

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Alexander Belyaev 32 Decoding the nature of DM

Probing DM properties at the LHC

The idea is to probe DM operators with different DM spin using the shape missing transverse momentum (MET)

we use the EFT approach: simplicity and model independence explore the complete set of DIM5/DIM6 operators involving two SM quarks (gluons) and two DM particles consider DM with spin=0, 1/2, 1 use mono-jet signature at the LHC

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Alexander Belyaev 33 Decoding the nature of DM

Vector mediator Vector mediator

?

Scalar mediator Scalar mediator Scalar mediator

Vector mediator

Scalar mediator Scalar mediator

C5,C5A D1T-D4T D1-D4, D5-D8

Mapping EFT operators to simplified models

,

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Alexander Belyaev 34 Decoding the nature of DM

Mono-jet diagrams from EFT operators

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Alexander Belyaev 35 Decoding the nature of DM

AB, Panizzi, Pukhov, Thomas arXiv:1610.07545 arXiv:1610.07545

scalar DM fermion DM vector DM

Missing ET (MET) distributions: the large range of slopes

MDM=100 GeV,

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Alexander Belyaev 36 Decoding the nature of DM

[C1] [D1] [V1] [C3] [D5] [D9] [V5]

MET distributions are the same for the fixed mass of DM pair [M(DM,DM)] & fixed SM operator With the increase of M(DM,DM), MET slope decreases (PDF effect)

Properties of MET distributions:

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Alexander Belyaev 37 Decoding the nature of DM

DM DM

q q

for pT

T(g) increase

D (x1 x2)/(x1 x2) is large and MET slope is steep

MET distributions are the same for the fixed mass of DM pair [M(DM,DM)] & fixed SM operator With the increase of M(DM,DM), MET slope decreases (PDF effect)

Properties of MET distributions for small and large M(DM,DM)

small M(DM,DM)

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Alexander Belyaev 38 Decoding the nature of DM

DM DM

q q

small M(DM,DM)

for pT

T(g) increase

D (x1 x2)/(x1 x2) is large and MET slope is steep

DM DM

q q g

large M(DM,DM)

for pT

T(g) increase

D (x1 x2)/(x1 x2) is small and MET slope is gradual

MET distributions are the same for the fixed mass of DM pair [M(DM,DM)] & fixed SM operator With the increase of M(DM,DM), MET slope decreases (PDF effect)

Properties of MET distributions for small and large M(DM,DM)

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Alexander Belyaev 39 Decoding the nature of DM

Distinguishing DM operators/theories

The flatter MET shapes The harder M(DM,DM) distributions

arXiv:1610.07545

➪projection for 300 fb-1: some operators C1-C2,C5-C6,D9-D10,V1-V2,V3-V4,V5-V6 and V11- 12 can be distinguished from each other ➪Application beyond EFT: when the DM mediator is not produced on-the-mass-shell and MDMDM is not fixed: t-channel mediator or mediators with mass below 2MDM

  • perator energy dependence → MDMDM shape → MET shape
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Alexander Belyaev 40 Decoding the nature of DM

scalar DM fermion DM vector DM

LanHEP→ CalcHEP→ LHE→ CheckMATE

ATLAS@13 TeV, 1604.07773 analysis cuts

LHC@13TeV reach projected 100 fb-1

AB, Panizzi, Pukhov, Thomas arXiv:1610.07545 arXiv:1610.07545

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Alexander Belyaev 41 Decoding the nature of DM

Distinguishing the DM operators: c2 for pairs of DM operators

: if c2>9.48 (95%CL for 4 DOF) –

  • perators can be distinguished!
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Alexander Belyaev 42 Dark Matter Characterisation at the LHC

Distinguishing the DM operators: c2 for pairs of DM operators

: if c2>9.48 (95%CL for 4 DOF) –

  • perators can be distinguished!
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Alexander Belyaev 43 Decoding the nature of DM

  • r

Importance of the operator running in the DM DD ↔ Collider interplay

In case of axial operators, e.g . couplings cV

(q) arise due to the running of the wilson coefficient cA (q)

leading to sizable constraints on the DM DD constraints

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Alexander Belyaev 44 Decoding the nature of DM

  • r

Importance of the operator running in the DM DD ↔ Collider interplay

In case of axial operators, e.g . cA

(u), cA (d), cV (u), cV (d)=(1,1,0,0)[1TeV] → (1.1, 1.1, 0.04, -0.07)[1GeV]

couplings cV

(q) arise due to the running of the wilson coefficient cA (q)

leading to sizable constraints on the DM DD constraints

runDM program (github.com/bradkav/runDM) by D’Eramo, Kavanagh Panci

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Alexander Belyaev 45 Decoding the nature of DM

  • r

Importance of the operator running in the DM DD ↔ Collider interplay

In case of axial operators, e.g . cA

(u), cA (d), cV (u), cV (d)=(1,1,0,0)[1TeV] → (1.1, 1.1, 0.04, -0.07)[1GeV]

runDM program (github.com/bradkav/runDM) by D’Eramo, Kavanagh Panci AB, Bertuzzo, Caniu, di Cortona, Eboli, Iocco, Pukhov 2018

couplings cV

(q) arise due to the running of the wilson coefficient cA (q)

leading to sizable constraints on the DM DD constraints

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Alexander Belyaev 46 Decoding the nature of DM

DM DD ↔ Collider interplay

AB, Bertuzzo, Caniu, di Cortona, Eboli, Iocco, Pukhov 2018

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Alexander Belyaev 47 Decoding the nature of DM

DM DD ↔ Collider interplay

AB, Bertuzzo, Caniu, di Cortona, Eboli, Iocco, Pukhov 2018

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Alexander Belyaev 48 Decoding the nature of DM

Beyond the EFT

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Alexander Belyaev 49 Decoding the nature of DM

There is no limit on the LSP mass if the mass of strongly interacting SUSY particles above ~ 1.9 TeV

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Alexander Belyaev 50 Decoding the nature of DM

detector

High PT jet Large missing PT (2c0

1)

process

High PT g

The most challenging case takes place when only c0

1,2 and c± are accessible at

the LHC, and the mass gap between them is not enough for leptonic signatures The only way to probe CHS is a mono-jet signature [ “Where the Sidewalk Ends? ...” Alves, Izaguirre,Wacker '11] , which has been used in studies on compressed SUSY spectra, e.g. Dreiner,Kramer,Tattersall '12; Han,Kobakhidze,Liu,Saavedra,Wu'13; Han,Kribs,Martin,Menon '14

SUSY Compressed Mass Spectrum scenario

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Alexander Belyaev 51 Decoding the nature of DM

Signal vs Background

difference in rates is pessimistic ... but the difference in shapes is encouraging: large DM mass → biger M(DM,DM) → flatter MET Signal and Zj background pT

j distributions for the 13 TeV LHC

normalised signal and Zj background distributions S and BG number of events for 100 fb-1

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Alexander Belyaev 52 Decoding the nature of DM

LHC/DM direct detection sensitivity

AB, Barducci,Bharucha,Porod,Sanz JHEP, 1504.02472

  • SUSY DM, can be around the corner (~100 GeV), but it is hard to detect it!
  • Great complementarity of DD and LHC for small DM (natural)SUSY region
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Alexander Belyaev 53 Decoding the nature of DM

Beyond monojet signature

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Alexander Belyaev 54 Decoding the nature of DM

Beyond the mono-jet signature

Current LHC reach with tt+ MET signature based on ATLAS_CONF_2016_050 results

Example of the vector resonance in the Composite Higgs model: Z'→ TT→ t t DM DM signature

Flacke, Jaine, Schaefers, AB, 2017

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Alexander Belyaev 55 Decoding the nature of DM

The role of Z' vs QCD for pp→ TT→ t t DM DM

arXiv: 1707.07000

Z' + QCD TT production

➪LHC is probing now DM and top partner masses up to about 0.9 and 1.5 TeV respectively ➪bounds from QCD production alone are extended by ~ factor of two ➪DM DD rates are loop-suppressed

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Alexander Belyaev 56 Decoding the nature of DM

Disappearing Charged Tracks (DCT): VDM as an example

The small mass gap (~ pion mass) between DM and its charged partner will lead to the disappearing charge tracks signatures

AB, Cacciapaglia, McKay, Martin, Zerwekh ‘18

V0 and V+ which are degenerate at tree- level are split due to the quantum corrections

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Alexander Belyaev 57 Decoding the nature of DM

Collider sensitivity to VDM mass

Using ATLAS arXiv:1712.02118 for LHC interpretation and Mahbubani,Schwaller, Zurita ArXiv:1703.05327 For 100 TeV FCC projections

0.06ns

The life-time should be properly evaluated using W-pion mixing (otherwise overestimated by factor of 10)

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Alexander Belyaev 58 Decoding the nature of DM

Collider sensitivity to VDM mass

Current bound from LHC on DM mass from the minimal vector triplet model: 1.3 TeV ! 100 TeV FCC will cover DM mass beyond 4TeV: will discover or close the model

AB, Cacciapaglia, McKay, Martin, Zerwekh arXiv:1808.10464

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Alexander Belyaev 59 Decoding the nature of DM

Decoding the nature of DM at the ILC

muon spectrum from the models with scalar and fermion DM

e+e- → D+ D- → DM DM W+ W- → DM DM jj m n

AB, Ginzburg, Locke, Freegard, Hosken, Pukhov preliminary

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Alexander Belyaev 60 Decoding the nature of DM

Decoding Problem: Data → Theory link

probably the most challenging problem to solve – the inverse problem of decoding of the underlying theory from signal

requires database of models, database of signatures

requires smart procedure based on machine learning of matching signal from data with the pattern of the signal from data

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Alexander Belyaev 61 Decoding the nature of DM

probably the most challenging problem to solve – the inverse problem of decoding of the underlying theory from signal

requires database of models, database of signatures

requires smart procedure based on machine learning of matching signal from data with the pattern of the signal from data

HEPMDB (High Energy Physics Model Database) was created in 2011 hepmdb.soton.ac.uk

convenient centralized storage environment for HEP models

it allows to evaluate the LHC predictions and perform event generation using CalcHEP, Madgraph for any model stored in the database

you can upload their own model and perform simulation

Decoding Problem: Data → Theory link

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Alexander Belyaev 62 Decoding the nature of DM

probably the most challenging problem to solve – the inverse problem of decoding of the underlying theory from signal

requires database of models, database of signatures

requires smart procedure based on machine learning of matching signal from data with the pattern of the signal from data

HEPMDB (High Energy Physics Model Database) was created in 2011 hepmdb.soton.ac.uk

convenient centralized storage environment for HEP models

it allows to evaluate the LHC predictions and perform event generation using CalcHEP, Madgraph for any model stored in the database

you can upload there your own model and perform simulation

As a HEPMDB spin-off the PhenoData project was created hepmdb.soton.ac.uk/phenodata

stores data (digitized curves from figures, tables etc) from those HEP papers which did not provide data in arXiv or HEPData

has an easy search interface and paper identification via arXiv, DOI or preprint numbers

Decoding Problem: Data → Theory link

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Alexander Belyaev 63 Decoding the nature of DM

➪DM DD detection provides a very powerful probe of DM theory space – in general provides DM mass probe beyond the collider reach ➪Colliders – provide DM detection power in the region “blind” for DM DD, typically below 1 TeV ➪Several ways to decode DM nature from the signal which we hope to

  • bserve soon (slopes of MET, cross sections, signatures, … )

➪New prospects: new DD experiments, new ideas, prospects for directional DM detection, new signatures at colliders (VFB, LL, …), future colliders (great potential of ILC and FCC) ➪Great synergy of collider and non-collider experiments (DD, CMB, relic density)

Summary

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Alexander Belyaev 64 Decoding the nature of DM

Thank you!

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Alexander Belyaev 65 Decoding the nature of DM

Backup Slides

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Alexander Belyaev 66 Decoding the nature of DM

DIM5/6 operators (spin 0,1/2,1)

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Alexander Belyaev 67 Decoding the nature of DM

Vector mediator Vector mediator

?

Scalar mediator Scalar mediator Scalar mediator

Vector mediator

Scalar mediator Scalar mediator

C5,C5A C1 D1T-D4T D1-D4, C3 D5-D8

Mapping EFT operators to simplified models

, D9,D10 [

  • ]

8

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Alexander Belyaev 68 Decoding the nature of DM

On the other hand, M(DM,DM) distributions, defined by the EFT operators are different!

SDM FDM VDM

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Alexander Belyaev 69 Decoding the nature of DM

DM DD ↔ Collider interplay

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Alexander Belyaev 70 Decoding the nature of DM

DM DD: directional detection – going beyond the neutrino floor

The idea is to measure both the energy and the direction of the recoil Most mature technology is the gaseous Time Projection Chamber (TPC) : DRIFT, MIMAC, DMTPC, NEWAGE, D3 Detecting recoil tracks in nuclear emulsion (e.g. NEWS experiment) Aleksandrov et al. [1604.04199] Directional detection is HARD, But it is also very POWERFUL.

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Alexander Belyaev 71 Decoding the nature of DM

Relation of the actual dimension (D) and the naive one (d) for VDM operators

we suggest a new parametrisation of VDM operators: since the energy E and the collider limit on L are of the same order, it is natural to use an additional MDM/L factor for each power of E/MDM enhancement, so collider limits are not artificially enhanced [~100 TeV !!! for MDM =1 GeV, see Kumar, Marfatia, Yaylali 1508.04466] and will be of the same order as limits for other operators Dictionary between limits on L in different parametrisations:

and

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Alexander Belyaev 72 Decoding the nature of DM

Distinguishing DM operators

MET cut (GeV) →

250 300 350 400 500 600 700

# of events consistent with 95% CL

  • perator energy dependence → MDMDM shape → MET shape
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Alexander Belyaev 73 Decoding the nature of DM

On the BG uncertainty

http://cms-results.web.cern.ch/cms-results/public-results/preliminary-results/EXO-16-013/#AddFig CMS-PAS-EXO-16-013

The BG is statistically driven, e.g. pp-> Zj → nnj BG is defined from the pp → Zj → l+l-j one

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Alexander Belyaev 74 Decoding the nature of DM

Complementarity of LHC and non-LHC DM searches

for the model with Vector Resonances, Top Partners and Scalar DM

arXiv: 1707.07000 QCD TT production

  • nly

TT→ t t DM DM

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Alexander Belyaev 75 Decoding the nature of DM

LHC@13TeV Reach for spin 0 and ½ DM

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Alexander Belyaev 76 Decoding the nature of DM

LHC@13TeV Reach for spin 1 DM

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Alexander Belyaev 77 Decoding the nature of DM

Disappearing Charged Tracks from DM

The small mass gap between (~ pion mass) DM and its charged partner will lead to the disappearing charge tracks The life-time should be properly evaluated using W-pion mixing