KnE Energy | The 3rd International Conference on Particle Physics and Astrophysics (ICPPA) | pages: 202–209

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and

1. Introduction

The neutrinoless double beta decay ( 0νββ ) is a hypothetical lepton-number-violating nuclear transition predicted by several extensions of the Standard Model of particle physics. Its detection would prove that neutrinos have a Majorana mass component [1,2] and that lepton number is not conserved, thus providing a possible answer to the matter-antimatter asymmetry in the Universe and the origin of neutrino masses [3,4,5].

Searches for 0νββ are ongoing in a number of experiment around the world using different nuclei as 76 Ge [6,7], 136 Xe [8,9,10] and 130 Te [11,12]. The experimental signature of 0νββ is a peak in the distribution of the energy sum of two electrons at the Q-value of the decay ( Qββ ). Typically only a few signal counts per kg per year are expected: therefore a very strong suppression of all background sources and a high energy resolution are required.

2. The GERDA experiment

The GERDA experiment [13], located at the underground Laboratori Nazionali del Gran Sasso (LNGS) of INFN in Italy, operates bare high-pure germanium detectors (HPGe) in liquid argon (LAr), which cools the detectors to their operating temperature of about 90 K and shields them from external radiation. The 64 m 3 LAr cryostat is contained in a 590 m 3 water tank, filled with ultra-pure water and equipped with photomultipliers, thus acting both as Cerenkov veto and additional shield. On the top of the water tank a clean room with a glove box and a lock is used for the assembly of HPGe detectors into strings. The HPGes are arranged in an array of 6 strings hosting detectors enriched in 76 Ge ( enr Ge): 7 coaxial detectors from the former Heidelberg-Moscow [14] and IGEX [15] experiments, and 30 newly developed Broad Energy germanium (BEGe) detectors [16] featuring superior pulse shape discrimination performance [17,18]. The detector array is complemented with a central string instrumented with three coaxial detectors made from germanium of natural isotopic composition. In Phase II, the cylindrical volume around the detector strings is instrumented with a curtain of wavelength-shifting fibres read out at both ends with 90 silicon photomultipliers (SiPMs). Sixteen low-background photomultipliers (PMTs) are mounted below and above of the HPGe array.

All Ge detectors are connected to low radioactivity charge sensitive amplifiers. The charge signal traces are digitized with a 100 MHz sampling rate and a total window of 160 μ s. Data are stored on disk and analyzed offline using the procedure described in [19,20].

3. Data taking and event selection

GERDA is taking data since 2011. Data from the first phase of GERDA (Phase I) gave no positive indication of the 0νββ decay with an exposure of about 21.6 kg · yr and a background index at the Qββ = ( 2039.061±0.007 ) keV of 10-2 cts/(keV · kg · yr). A lower limit on the half-life of the process of T1/20ν >2.1·1025 yr (90 % C.L.) was set [19]. The second phase (Phase II), is ongoing since December 2015 and initial results were released in June 2016 with 10.8 kg · yr of total exposure and a background index of 10-3 cts/(keV · kg · yr) [6]. In June 2017 new data collected up to April 15th 2017 have been fully validated and analyzed for a total exposure of 34.4 kg · yr of enr Ge (18.2 kg · yr from BEGe detectors and 16.2 kg · yr from coaxial detectors) [21].

The offline data analysis flow foresees a blind approach: events with a reconstructed energy in the interval Qββ ± 25 keV are not analysed but only stored on disk. After the entire analysis procedures and parameters have been frozen, these blinded events are processed.

Unphysical events, originating from electrical discharges or bursts of noise, are rejected by a set of multi-parametric cuts based on the flatness of the baseline, polarity and time structure of the pulse. Physical events at Qββ are accepted with an efficiency greater than 99.9 % while no unphysical event survives the cuts above 1.6 MeV.

In 92 % of 0νββ decays occurring in the active detector volume, the total 0νββ energy is detected in that detector. Therefore multiple detector coincidences are discarded as background events. In order to discriminate time-correlated decays from primordial radioisotopes, such as the radon progenies 214 Bi and 214 Po, two consecutive candidate events within 1 ms are rejected. Candidate events are also rejected if a muon trigger occurred within 10 μ s before a germanium detector trigger or if any of the LAr light detectors record a signal of amplitude above 50 % of the expectation for a single photo-electron within 5 μ s from the germanium trigger.

The deposited energy is reconstructed with an improved digital filter [22] optimized for each detector and each calibration. The energy scale and resolution is set by taking weekly calibration with 228 Th sources. The stability of the scale is continuously monitored by injecting charge pulses (test pulses) with a rate of 0.05 Hz and, weekly, by checking the shift of the position of the 2615 keV γ line between two consecutive calibration (Fig. figcala). The average resolution at Qββ , evaluated by using the calibration data, is shown in Fig. figcalb; for coaxial detectors the width of the strongest γ lines in the physics data (1460 keV from 40 K and 1525 keV from 42 K) is found to be 0.5 keV larger than expected, probably due to gain instabilities in the corresponding readout channels between calibrations. The effect is accounted for by including a correction term; the average resolution at Qββ is 3.90(7) keV and 2.93(6) keV FWHM for the enr Ge coaxial and BEGe detectors, respectively.

Figure 1

(a) Average shift of the 2615 keV γ -ray line between consecutive calibrations. The error bars represent the standard deviation of the shifts of the individual detectors. (b) Average energy resolution for γ lines observed in calibration data and in physics data, for the BEGe and coaxial detectors. The inset displays a zoom of the γ lines at 1460 keV ( 40 K) and 1525 keV ( 42 K) in physics data, and a zoom of the 2615 keV line from calibration data.





Due to the short range of electrons in germanium ( 1 mm), 0νββ decays produce a localized energy deposit. The time profile of the Ge current signal can be used to disentangle 0νββ decays (single-site events, SSE) from background events such as γ -rays, which mainly interact via Compton scattering with an average free path of 1 cm (multi-site events, MSE), or external α / β -rays, which deposit their energy on the detector surface. The geometry of the BEGe detectors allows the application of a simple mono-parametric Pulse Shape Discrimination (PSD) technique based on the maximum of the detector current pulse A normalized to the total energy E [17,18][23]. The cut on A/E allows to reject >90% of ( γ -like) MSEs and basically all α -like surface events, with a 0νββ selection efficiency of (87±2) %. For coaxial detectors two neural network algorithms (ANN) are applied to discriminate SSEs from MSEs and from α surface events [18] with a combined selection efficiency for 0νββ decays of (79±5) %.

4. Statistical analysis and results

In June 2017, data from the BEGe detectors taken between June 1, 2016 and April 15, 2017 has been unblinded, providing an additional exposure of 12.4 kg · yr with respect to [6]. Two extra events passing all selection cuts are found in the blinded energy region; both of them being more than 15 keV away from Qββ (namely >10σ ) they cannot be attributed to 0νββ decay. Due to a recently identified background population not efficiently rejected by ANN PSD, data from coaxial detectors (11.2 kg · yr) were not unblinded. It will be unblinded in a future data release, when a new cut is developed to suppress this background. The background in the signal region is 10-3 cts/(keV · kg · yr) for BEGe detectors and 2.7 × 10-3 cts/(keV · kg · yr) for coaxials. The energy spectra around Qββ for Phase I, Phase II coaxial detectors and Phase II BEGe detectors (after all cuts) are shown in Fig. figroizoom.

The total exposure available for analysis is (471.1±8.5) mol · yr of 76 Ge. Both a frequentist and a Bayesian analysis, based on an unbinned extended likelihood function described in the Methods Section of Ref. [6], is performed. The fit function is a flat distribution for the background and a Gaussian centered at Qββ with a width according to the resolution for a possible 0νββ signal. The signal strength S = 1 /T1/20ν is calculated for each data set (both for Phase I and Phase II, for coaxial and BEGe detector respectively) according to its exposure and efficiency while the inverse half-life 1/T is a common free parameter. The analysis accounts for the systematic uncertainties due to efficiencies and energy resolutions, and to a possible offset in the energy scale. The limit on the half-life of 76 Ge is T1/20ν>8.0·1025 yr (90% CL) (frequentist) and T1/20ν>5.1·1025 yr (Bayesian), while the median sensitivity for the 90% CL lower limit of T1/20ν is 5.8·1025 yr (frequentist) and T1/20ν>4.5·1025 yr (Bayesian).

Figure 2

Energy spectra around Qββ for Phase I, Phase II coaxial detectors and Phase II BEGe detectors after all cuts. The binning is 2 keV. The blue lines show the hypothetical 0νββ signal for T1/20ν=8.0·1025 yr, sitting on the constant background.


5. Conclusions

The GERDA experiment is currently taking data. The ambitious design goal for the background level of 10-3 cts/(keV · kg · yr) was fulfilled, thus, making Gerda the first “background-free” experiment for the whole design exposure; the sensitivity is therefore expected to grow linearly with the exposure and the median sensitivity is expected to reach 10 26 yr within 2018. At present, thanks to the powerful pulse shape discrimination of BEGe detectors and to the detection of the argon scintillation light, GERDA has reached the world-best background index (BI) at Qββ if weighted with the energy resolution of the detectors.

The excellent performances in terms of background index and energy resolution motivates a future extension of the program in a medium term time scale. The LEGEND collaboration aims to build a 200 kg enriched germanium experiment using the GERDA cryostat. Such an experiment would remain background-free up to an exposure of 1000 kg · yr provided the background can be further reduced by a factor 5-10;; thus LEGEND-200 [24] would allow to reach a half-life of 10 27 yr. The 200 kg project is conceived as a first step towards a more ambitious 1-ton experiment that would allow to reach a sensitivity of 10 28 yr, thus, fully covering the inverted hierarchy region in ten years of data taking.



J. Schechter J. W. F. Valle Neutrinoless double-β decay in su(2) x u(1) theoriesPhysical Review D: Particles, Fields, Gravitation and Cosmology19822511, article 295110.1103/PhysRevD.25.2951


M. Duerr M. Lindner A. Merle On the quantitative impact of the Schechter-Valle theoremJournal of High Energy Physics201120116, article 09110.1007/JHEP06(2011)091Zbl1298.81419


S. Davidson E. Nardi Y. Nir LeptogenesisPhysics Reports20084664-51051772-s2.0-5014911994910.1016/j.physrep.2008.06.002


Mohapatra R N et al. 2007 Rept. Prog. Phys. 70 1757–1867


Päs H and Rodejohann W 2015 New J. Phys. 17 115010


Agostini M et al. (GERDA) 2017 Nature 544 47


Guiseppe V E et al. 2017 AIP Conf. Proc. 1894 020010 (Preprint 1708.07562)


J. B. Albert D. J. Auty P. S. Barbeau Search for Majorana neutrinos with the first two years of EXO-200 dataNature201451022923410.1038/nature13432


Gando A et al. (KamLAND-Zen) 2016 Phys. Rev. Lett. 117 082503


Albert J et al. (EXO-200) 2017 (Preprint 1707.08707)


Alfonso K et al. (CUORE) 2015 Phys. Rev. Lett. 115 102502


Andringa S et al. (SNO+) 2015 Adv. High Energy Phys. 2016 6194250


Ackermann K H et al. (GERDA) 2013 Eur. Phys. J. C73 2330


Klapdor-Kleingrothaus H V et al. (Heidelberg-Moscow) 2001 Eur. Phys. J. A12 147–154


Aalseth C E et al. (IGEX) 2002 Phys. Rev. D65 092007


Agostini M et al. (GERDA) 2015 Eur. Phys. J. C75 39


Budjáš D, Barnabé Heider M, Chkvorets O, Khanbekov N and Schönert S 2009 JINST 4 P10007


Agostini M et al. (GERDA) 2013 Eur. Phys. J. C73 2583


Agostini M et al. (GERDA) 2013 Phys. Rev. Lett. 111 122503


Agostini M, Pandola L and Zavarise P 2012 J. Phys. Conf. Ser. 368 012047


Agostini M et al. (GERDA) 2017 (Preprint 1710.07776)


Agostini M et al. (GERDA) 2015 Eur. Phys. J. C75 255


Agostini M, Bellotti E, Brugnera R, Cattadori C M, D'Andragora A, di Vacri A, Garfagnini A, Laubenstein M, Pandola L and Ur C A 2011 JINST 6 P04005


Abgrall N et al. (LEGEND) 2017 AIP Conf. Proc. 1894 020027 (Preprint 1709.01980)



  • Downloads 15
  • Views 183



ISSN: 2413-5453