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Strongly interacting dark Strongly interacting dark matter doesn’t explain the matter doesn’t explain the DAMA signal DAMA signal Maxim Laletin in collaboration with J.R. Cudell Star Institute Université de Liège 8 th COSPA Meeting 10/11/2017

Strongly interacting dark matter doesn’t explain the DAMA ... · Composite dark matter Signifcant elastic cross sections (~ 10-26 cm2) Tiny recoil energies (slow down before the

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Page 1: Strongly interacting dark matter doesn’t explain the DAMA ... · Composite dark matter Signifcant elastic cross sections (~ 10-26 cm2) Tiny recoil energies (slow down before the

Strongly interacting dark Strongly interacting dark matter doesn’t explain the matter doesn’t explain the

DAMA signalDAMA signal

Maxim Laletinin collaboration with J.R. Cudell

Star InstituteUniversité de Liège

8th COSPA Meeting10/11/2017

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Maxim Laletin (ULiege) 2

Direct detection puzzle

J. Cooley, Phys.Dark Univ. 4, 2014

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Maxim Laletin (ULiege) 3

DAMA Experiment

Annual modulation of the signal

9.3 σ C.L.9.3 σ C.L.

DAMA/LIBRA250 kg NaI(Tl)

1.33 ton*yr~ 103 counts per day

LNGS, Gran SassoLNGS, Gran Sasso

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Maxim Laletin (ULiege) 4

Explanations● Background neutrons● Muon-induced neutrons● Neutrino-induced neutrons

However, these explanations don’t workHowever, these explanations don’t work

● “No role for neutrons, muons and solar neutrinos in the DAMA annual modulation results”, Bernabei et al., Eur.Phys.J., 2014

● “Comment on "Fitting the annual modulation in DAMA with neutrons from muons and neutrinos''”, Barbeau et al., Phys.Rev.Lett., 2014

● “Can muon-induced backgrounds explain the DAMA data?”, Klinger and Kudryavtsev, J.Phys.Conf.Ser., 2016

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Maxim Laletin (ULiege) 5

Any room for dark matter?

● Resonant Dark Matter, Yang Bai, Patrick J. Fox (Fermilab) JHEP 0911 (2009) 052● Mirror dark matter interpretations of the DAMA, CoGeNT and CRESST-II

data, R. Foot Phys.Rev. D86, 2012● Inelastic dark matter with spin-dependent couplings to protons and

large modulation fractions in DAMA, Stefano Scopel, Kook-Hyun Yoon, JCAP 1602, 2016

Essentially, all these models assume that DAMA detector is somehow “special”,

so that there is no signal in other detectors

Yes, but not for simple WIMPs

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Maxim Laletin (ULiege) 6

Composite dark matter● Signifcant elastic cross sections (~ 10-26 cm2)● Tiny recoil energies (slow down before the

detector)● Produce the signal due to inelastic processes on

some special component of DAMA

● Composite Dark Matter and Puzzles of Dark Matter Searches, M. Khlopov, A. Mayorov, E. Soldatov, Int.J.Mod.Phys. D19 (2010)

● Milli-interacting dark matter, Q. Wallemacq, Phys. Rev. D 88 (2013)● Dark antiatoms explain DAMA, J.R. Cudell, Q. Wallemacq, JCAP 2015

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Maxim Laletin (ULiege) 7

Slowdown in the ground

Thermalization depth

The recoil energy on nuclei is tiny

DM looses energy after multiple collisions on terrestrial nuclei (mainly Si and O) and acquires the surrounding temperature (thermalizes)

Mean free path length

Number density of the medium (rock)

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Maxim Laletin (ULiege) 8

Diurnal modulation

One expects diurnal modulation for

SIMPs

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Maxim Laletin (ULiege) 9

Diurnal modulation

DAMA data Expected for WIMPs

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Maxim Laletin (ULiege) 10

Diurnal modulation

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Maxim Laletin (ULiege) 11

Propagation in the groundThe propagation can be described as diffusion with a drift due to gravity

Particle number density Source function

Difusion coefcient Drift velocity(related to the difusion coefcient

via Einstein relation)

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Maxim Laletin (ULiege) 12

“Flat-Earth” approximation

All the points on the surface are equal,so the only dimension that matters is Z

1D difusion equation

Slow difusion only takes place below the surfaceAbove the surface the difusion coefcient is 0

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Maxim Laletin (ULiege) 13

Density in the detectorGeneral solution of the diffusion equation in the unbounded space

with the Green’s function Depth distribution

Drift factor“Mirror” sink term

describes the leakageof particles into the air

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Maxim Laletin (ULiege) 14

Velocity distributionDark matter thermal velocity distribution

Can be translated intothe depth distribution

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Maxim Laletin (ULiege) 15

Constraints

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Maxim Laletin (ULiege) 16

Let’s study a particular set of parameters,M = 1 TeV

σ = 10-26 cm2

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Maxim Laletin (ULiege) 17

Density inside the detector

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Maxim Laletin (ULiege) 18

Density inside the detector

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Maxim Laletin (ULiege) 19

Reconstructing the signalInelastic cross section -

additional parameter that we use to normalize the signal

~ 10-3

The rate is than averaged over every day and the yearly average of the signal(background) is subtracted

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Maxim Laletin (ULiege) 20

Annual modulation

~ 100 days shift

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Maxim Laletin (ULiege) 21

Diurnal modulation

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Maxim Laletin (ULiege) 22

Other parameter valuesM = 100 GeV

σ = 10-26 cm2

Annual modulation

Diurnal modulation

~ 90 days shift

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Maxim Laletin (ULiege) 23

Other parameter valuesM = 100 TeV

σ = 6 10-24 cm2

Annual modulation

Diurnal modulation

~ 60 days shift

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Maxim Laletin (ULiege) 24

Realistic surface

DAMA is here Gran Sasso mountain

(Google Earth)

A more detailed picture includes a complex realistic surface

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Maxim Laletin (ULiege) 25

Realistic surfacePreliminaryPreliminary

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Maxim Laletin (ULiege) 26

Conclusions● The effects of propagation rule out some dark matter

models explaining the DAMA results with strongly interacting massive particles;

● Both annual and diurnal modulations cannot be reproduced;● The effects of “bouncing” particles needs to be studied,

however a signifcant improvement of the ft is not expected; ● DAMA results will be tested in a series of experiments:

ANAIS, COSINE-100, SABRE, COSINUS and so on.

Thank you for attention!

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Maxim Laletin (ULiege) 27

Backup

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Maxim Laletin (ULiege) 28

Constraints on SIMPs

Erickcek+, Phys. Rev. D 2007, 0704.0794

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Maxim Laletin (ULiege) 29

XENON1T (2017)

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Maxim Laletin (ULiege) 30

Signal comparison

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WIMP Signalaround annual

maximum

SIMP Signalaround annual

maximum

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Maxim Laletin (ULiege) 32

Signal reconstruction

Averaged over each day(annual modulation)or each hour of every day during the year

(diurnal modulation)

Averaged over the year

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Maxim Laletin (ULiege) 33

Dark antiatoms● Dark antiproton and dark positron● Dark photon can “convert” to ordinary photon● Interacts strongly with “our world”● Couple to heavy elements (Thalium in DAMA)● Emit X-rays, which produce electron recoils

J.R. Cudell, Q. Wallemacq, JCAP 2015

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Maxim Laletin (ULiege) 34

“Bouncing” SIMPs

However, we do not expect this to drastically change our conclusion