Virtual depth by active background suppression: revisiting the cosmic muon induced background of Gerda Phase II

In-situ production of radioisotopes by cosmic muon interactions may generate a non-negligible background for deep underground rare event searches. Previous Monte Carlo studies for the Gerda experiment at Lngs identified the delayed decays of 77\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{77}$$\end{document}Ge and its metastable state 77m\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{77m}$$\end{document}Ge as dominant cosmogenic background in the search for neutrinoless double beta decay of 76\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{76}$$\end{document}Ge. This might limit the sensitivity of next generation experiments aiming for increased 76\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{76}$$\end{document}Ge mass at background-free conditions and thereby define a minimum depth requirement. A re-evaluation of the 77(m)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{77(m)}$$\end{document}Ge background for the Gerda experiment has been carried out by a set of Monte Carlo simulations. The obtained 77(m)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{77(m)}$$\end{document}Ge production rate is (0.21±0.01\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$0.21\pm 0.01$$\end{document}) nuclei/(kg·\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\cdot $$\end{document}year). After application of state-of-the-art active background suppression techniques and simple delayed coincidence cuts this corresponds to a background contribution of (2.7±0.3)×10-6\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$(2.7\pm 0.3)\times 10^{-6}$$\end{document} cts/(keV·\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\cdot $$\end{document}kg·\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\cdot $$\end{document}year). The suppression achieved by this strategy equals an effective muon flux reduction of more than one order of magnitude. This virtual depth increase opens the way for next generation rare event searches.


Introduction
In-situ production of radioactive isotopes by cosmic muon interactions constitutes a non-negligible background for rare event searches and may define a minimum depth for experiments aiming for ultra-low backgrounds [1]. In [2] the muon induced background for the Gerda (GErmanium Detector Array) experiment [3] at Lngs (Laboratori Nazionali del Gran Sasso) of Infn was studied. The delayed decays of 77 Ge and its isomeric state 77m Ge were identified as dominant cosmogenic background in Gerda's search for neutrinoless double beta (0νββ) decay of 76 Ge. 77(m) Ge is formed by neua e-mail: christoph.wiesinger@tum.de tron capture on the double beta isotope 76 Ge itself. 1 A background contribution of (1.1 ± 0.2) × 10 −4 cts/(keV·kg·year) at 0νββ relevant energies before active background rejection cuts was reported. This is well below the background of Gerda Phase II, but might constitute a significant fraction of the background budget for the next generation experiment Legend (Large Enriched Germanium Experiment for Neutrinoless ββ Decay) [4]. Legend is aiming to perform a background-free search for 0νββ decay with increased 76 Ge mass.
In this work a re-evaluation of the 77(m) Ge background in Gerda is carried out by a set of Monte Carlo simulations. They use the actual Phase II geometry and up-todate 76 Ge neutron capture cross section data. A description of the Gerda setup and its Monte Carlo implementation can be found in Sect. 2. Results from 77 Ge and 77m Ge decay simulations and the impact of active background suppression techniques are shown in Sect. 3. The production of 77(m) Ge by cosmic muon induced neutrons is discussed in Sect. 4. Prospects for reduction by delayed coincidence cuts are described in Sect. 5. In Sect. 6 minor cosmogenic background contributions from other sources are discussed briefly. Final conclusions on the feasibility of a next generation 76 Ge experiment at Lngs exploiting the Gerda passive and active shielding approach are drawn in Sect. 7.

GERDA
Gerda is searching for the 0νββ decay of 76 Ge. High purity germanium (HPGe) detectors enriched in 76 Ge constitute simultaneously source and detector for the search of the mono-energetic line at the Q-value of 2039 keV (Q ββ ). Gerda is situated in Hall A of the Lngs underground laboratory of Infn in Italy. Lngs provides an overburden of 3500 m.w.e. and a residual muon flux of ∼ 1.25 m −2 h −1 . The outermost part of the experiment is a 590 m 3 water tank. The water efficiently acts as neutron absorber and is equipped with photomultiplier tubes (PMTs) to serve as Cherenkov veto for cosmic muons. The muon veto system is completed by plastic scintillator panels on top of the experiment. The water tank surrounds a cryostat filled with 64 m 3 of liquid argon (LAr). The instrumentation is lowered into this cryostat from a clean room on top of the experiment via an airtight lock system. The first phase of Gerda (Phase I) was performed between 2011 and 2013 [5]. In Phase II 40 HPGe detectors are operated in a 7 string array configuration. 37 of them are made from isotopically enriched germanium material with an enrichment fraction of 87% 76 Ge. They constitute a detector mass of 35.6 kg. The 3 remaining detectors feature natural isotopic composition. The LAr volume around the array is instrumented with wavelength shifting fibers coupled to silicon photomultipliers (SiPMs) [6,7] and low-activity PMTs. The ability to detect scintillation light allows to reject backgrounds with coincident energy release in HPGe detectors and LAr [8]. Results from Phase II were published in [9,10]. A detailed description of the Gerda Phase II setup can be found in [11].

Monte Carlo implementation
The Monte Carlo simulations for this work were carried out by the Geant4-based [12][13][14] MaGe framework [15]. It is jointly developed and maintained by the Gerda and Majorana [16] collaborations. The Gerda Phase II implementation includes all relevant components of the experiment as well as the rock surroundings of Hall A at Lngs. The simulations in this work are performed with MaGe built against Geant4 10.3. The default physics list of MaGe is used. 2 It corresponds to the reference physics list QGSP_BERT_HP of Geant4. Inelastic interactions of nucleons and pions are simulated according to the theory-driven quark-gluon string (QGS) model above 20 GeV; according to the Fritiof (FTF) model between 10 and 20 GeV; and according to the Bertini cascade (BERT) model below 10 GeV. Interactions of neutrons below 20 MeV and down to thermal energies are described accurately by the high-precision data-driven models (NeutronHP) based on the evaluated ENDF/B-VII data libraries [17]. The specialized low-energy models based on the Livermore data library are used for the electromagnetic interactions of electrons and γ rays. The model for muonnuclear interaction is G4MuNuclearInteraction. This physics list has been shown to provide good performance in handling low-energy electromagnetic interactions as well as hadronic showers initiated by high-energy cosmic muons [15]. 2 Simulations with the reference Shielding physics list provided by Geant4 produced equal results.
The production of isotopes in muon induced cascades can be either due to the hadronic (or lepton-nuclear) interactions within the hadronic shower, or to secondary neutrons emerging from the shower. The former is the dominant mechanism for the production of nuclei (A,Z) "far away" with respect to the target nucleus (e.g. 60 Co production from Ge). The production of "nearby" nuclei is mostly ascribed to secondary neutron interactions, as radiative capture (n,γ ) and inelastic scattering (n,X), e.g. (n,p). This is the case of the most relevant species discussed in this paper, namely 77(m) Ge from 76 Ge, 41 Ar and 40 Cl from 40 Ar.
The evaluation of the neutron-mediated production yield involves two ingredients, namely the generation of neutrons from the muon induced showers and the neutron tracking down to their capture/interaction, which may happen at thermal energies. The capability of Geant4 to provide a realistic estimate of the muon induced neutron production in underground sites has been widely discussed in the literature (see e.g. [18][19][20]). The neutron yield predicted by Geant4 for muon induced interactions in a low-A target, as organic liquid scintillator, was found to agree with the experimental results from KamLAND within 10% [21]. As for neutron production in high-A materials, the recent work of [22,23] reports that Geant4 under-estimates it by a factor of 3-4 in Pb for cosmic muons at shallow depth ( E μ = 7 GeV). However, [20] shows that Geant4 slightly over-estimates the neutron production in Pb in a deep underground laboratory ( E μ = 260 GeV) by 25% and that the choice of the physics list has a < 5% impact. The weak dependency on the physics list was also observed in [15]: the differences in neutron yield from high-energy muons in metallic germanium were found to be within 15%. As the configuration in [20] is more representative of the muon energy spectrum at Lngs ( E μ = 270 GeV) than in [23], the systematic uncertainty on the muon-induced neutron production is taken to be 25%. This is also reasonably conservative, as the Gerda setup is composed entirely by low-A materials, with water and argon being the most relevant.
As mentioned above, the data-driven NeutronHP models based on the ENDF/B-VII data libraries are used for the tracking of neutrons below 20 MeV. The error due to the interpolation of adjacent data points is smaller than a few percent [24]. It has been shown in [25] that the agreement for the neutron propagation between Geant4 and the MCNPX code [26], which uses tabulated data from the alternative JENDL database [27], is better than 20%, and often within 10%. Taking also into account the study of [28], the global uncertainty for neutron propagation due to the Geant4 NeutronHP models is estimated here to be 20%. When combining the two terms in quadrature, the global systematic uncertainty for isotope production mediated by muon induced neutrons results Fig. 1 Left: simplified decay scheme for 77 Ge and 77m Ge. Both isotopes undergo β-decay to 77 As. 77m Ge undergoes mainly pure groundstate decay without the release of coincident γ 's. Middle/right: spectra for 77 Ge and 77m Ge decays in enriched detectors of Gerda Phase II. The reduction by consecutive application of active background rejec-tion techniques is shown. The spectra are normalized to represent the spectral contribution per decay, the binning is 20 keV. The inset shows the R 90 distribution for events around Q ββ . It is used to model the multi-site event rejection by PSD to be 35%, provided that the cross sections for the relevant isotopes are included in the ENDF/B-VII library. 3 The systematic uncertainty on the production yield is substantially larger for those nuclei that are mostly produced by other mechanisms which do not involve neutrons, as leptonuclear reactions, direct spallation or high-energy proton scattering. This can be up to a factor of four for germanium targets and for the product nuclei of interest for this work [29,30].

Active background rejection
Apart from passive background reduction in terms of graded passive shielding and extensive material selection efforts, active background rejection is a key feature of the Gerda experimental approach. The electrons released in 76 Ge double beta decay will deposit their energy within short range in one single site in one HPGe detector. Background events exhibiting a different topology can be efficiently rejected by the means of active background rejection techniques [31].
Events with simultaneous energy depositions in multiple HPGe detectors are rejected by detector anti-coincidence (AC). A realistic offline trigger threshold of 10 keV in the AC condition of simulated data is used. Analogously events with coincident energy deposition in the LAr surroundings are suppressed by the Phase II scintillation light read-out system (LAr veto). For the sake of computing power a simplified effective model is used. Events are rejected if a coincident energy deposition in the LAr volume contained by the light instrumentation exceeds 150 keV.
The finite drift time of charge carriers in HPGe detectors allows to discriminate events differing from single-site bulk energy depositions by pulse shape discrimination (PSD) [32]. The multi-site event rejection of PSD is modeled by a simple post-simulation parametrization described in [33]. The parameter R 90 , defined as the radius from the barycenter of energy depositions containing 90% of the deposited energy, is calculated per HPGe detector. Energy depositions exceeding a size of 2 mm in R 90 are classified as rejected. The signal acceptance for simulated 0νββ events with energy deposition at Q ββ is 97.3% (see inset in Fig. 1). This approximative model allows to draw fast and simple conclusions on the multi-site rejection performance by PSD without the need for sophisticated pulse shape simulations.
The parameters used in this simplified modeling of the active background rejection are chosen to represent a conservative estimate in comparison to experiences with the Gerda setup. Ongoing efforts for next generation of experiments aim for improved background suppression performance by e.g. increased LAr light yield, improved photon detection and low threshold/low noise HPGe detector read-out electronics. The obtained results hence represent a conservative baseline for future experiments.

Active suppression of 77(m) Ge decays
With a Q-value of about 2.7 MeV both the β-decays of 77 Ge and 77m Ge contribute to the background of experiments searching for 0νββ decay with 76 Ge. The simplified decay scheme is depicted in Fig. 1. The half-life is 11.2 h for 77 Ge and 53.7 s for 77m Ge [34]. With a probability of (19 ± 2)% 77m Ge undergoes internal transition to 77 Ge and emits a γ with 160 keV. The direct transition between the ground states of 77 Ge and of its daughter nucleus 77 As is spin-suppressed. All 77 Ge β-decays are followed by γ emission from deexcitation of 77 As excited states. A minimum of 195 keV corresponding to the first excited state of 77 As is released in coincidence. This results in a high chance to reduce this background by state-of-the-art active background rejection techniques. Vice-versa 77m Ge decays in (58 ± 4)% via pure ground-state decay without emitting additional γ 's. A single β released in the bulk of a HPGe detector represents a similar topology as double beta events. Hence, a large fraction of this background is expected to be irreducible by the current background rejection techniques based on prompt coincidences. Nevertheless, the comparably short half-life of 77m Ge opens up the possibility for rejection by delayed coincidence cuts as discussed in Sect. 5. 77 Ge and 77m Ge decays have been simulated in enriched HPGe detectors of the Gerda Phase II array. The obtained spectra are shown in Fig. 1. The inset shows the R 90 distribution in comparison with the single-site dominated distribution for 0νββ decays. As expected from decay scheme considerations, the suppression by active background rejection is large for 77 Ge only. The shape of the final spectrum after application of AC, LAr veto and PSD multi-site rejection reveals the contributions from β's to different levels of the 77 As daughter nucleus. Different γ emissions from subsequent de-excitations are visible in the unsuppressed spectrum prior cuts. Only minor suppression is achieved for 77m Ge. It is driven by a subdominant transition via the 215 keV state of 77 As. The unsuppressed 160 keV peak corresponds to the internal transition, the subsequent decay is taken into account in the 77 Ge spectrum.
The resulting spectral contributions at Q ββ ± 100 keV are summarized in Table 1. Generally β's are contained in a single detector. The dominance of β's in the 77m Ge energy release manifests in a larger initial contribution at Q ββ and less rejection power by active background suppression based on prompt coincidences.

Cosmic muon induced 77(m) Ge production
The cosmic muon induced production of radioactive isotopes was studied by the Monte Carlo simulation of muons impinging the Gerda setup. Their distribution in energy and direction was simulated with the Musun [35] Monte Carlo code and is shown in Fig. 2. The mean energy of the muons is 270 GeV. The azimuth and zenith angle distributions follow the profile of the Gran Sasso mountain. The code has been validated against measurements by the LVD experiment [36] situated next to Gerda in Hall A of the Lngs underground laboratory. In total 1 × 10 8 muons were released from a 12 × 12 × 13 m 3 sized box around the Gerda setup. 4 This corresponds to a lifetime of 43.4 years or 1544 kg·year of Gerda Phase II exposure.
Among other particles, neutrons are produced in various processes induced by cosmic muons. The main production channels are photon nuclear interactions and the production of secondary neutrons from inelastic neutron interactions. Figure 3 shows the spatial distribution of neutron production vertices. The muon induced neutron flux at the position of the HPGe detector array is 1.6 m −2 h −1 . This is less than the 5.7 m −2 h −1 obtained in [2]. The difference can be attributed to the updated Gerda Phase II setup with respect to the original design (notably, the different shape, dimensions and material of the cryostat) and to changes in Geant4. After scattering down in energy, neutrons end up to be absorbed in materials of the Gerda setup. The production vertices of neutrons eventually forming 77(m) Ge in the germanium detectors are highlighted in Fig. 3. Mainly neutrons generated in the LAr cryostat walls or in the LAr volume contribute to the 77(m) Ge production. The water tank efficiently shields the detector array from other neutrons. All muons initiating the production of 77(m) Ge point towards the cryostat volume. Proper tracking capability for muons might allow to identify muons associated with neutron production in the inner part of the experiment.
The cross section for neutron capture on 76 Ge has been recently measured at different energies [37][38][39]. The evaluations are based on the determination of γ intensities involved in the 77 Ge and 77m Ge decay. The directly accessible quantities are σ and σ m . The cross section σ includes the direct 77 Ge production cross section σ d and (19 ± 2)% of internal transitions from 77m Ge, whereas σ m describes the 77m Ge production only. The G4NDL library responsible for neutron capture on 76 Ge in Geant4 is based on ENDF/B-VII-1 tabulated data, which does not provide σ d + σ m for total 77(m) Ge production. The ratio of σ m to σ d + σ m measured at different neutron energies is shown in Fig. 4. With increasing neutron energy the cross sections favor 77 Ge over 77m Ge production, as higher neutron energies may result in higher excited states [39]. Considering the neutron energies involved in the insitu 77(m) Ge production a constant ratio for σ m to σ d + σ m of (50 ± 10)% is used in this analysis. This implies that the plain Geant4 cross section underestimates 77(m) Ge production by 68%. The Monte Carlo cross section σ MC was artificially increased in the performed simulation to account for this. It is depicted in Fig. 4. Measurements representing σ d + σ m agree reasonably well.
Neutron interaction cross-sections of materials in the germanium array vicinity define the spatial and temporal distribution of muon induced neutrons entering the array, especially at low neutron energies where the cross section for neutron capture on 40 Ar dominates. Folding the neutron distribution with the neutron capture on 76 Ge cross section the 77(m) Ge production rate was obtained. Figure 4 shows the resulting capture rate in neutron energy vs. time. A large fraction of the 77(m) Ge production appears to be prompt (< 10 µs) after the muon hits the experiment. Only the resonance at 550 eV has strong contribution to delayed captures. The cross section at thermal energies plays a minor role. The simulation yields a production rate of muon induced 77(m) Ge in Gerda of (0.21 ± 0.01) nuclei/(kg·year). It represents the main production channel 5 and allows verification in Gerda and next generation germanium experiments. 6 In combination with the results from Sect. 3 this leads to a background contribution of (1.5 ± 0.2) × 10 −6 cts/(keV·kg·year) from 77 Ge and (1.8 ± 0.4) × 10 −5 cts/(keV·kg·year) from 77m Ge. 7

77m Ge rejection by delayed coincidence
The strong single beta component of 77m Ge is irreducible with background rejection techniques based on prompt coincidences. However, the comparably short half-life of 53.7 s opens up possibilities to reduce this background by delayed coincidence cuts. Neutron capture leaves the daughter nucleus in a highly excited state, according to the available nuclear binding energy and level scheme. Its de-excitation results in the release of γ 's. In Geant4 this is represented by tabulated γ emission data [24]. According to Fig. 4 most captures on 76 Ge appear shortly after the actual muon is detected by the Gerda muon veto system. The read-out scheme will not allow to register separate events in muon veto and germanium detectors if within < 10 µs. Figure 5 shows the prompt single event multiplicity registered in the germanium detector array for muon events and for muon events with 77(m) Ge production. In addition to the prompt signal from the muon induced shower itself, the γ emission from inelastic neutron interactions in and around the array contributes to the enhanced multiplicity for the latter one. The efficiency to Fig. 4 Left: recent cross section data for 77 Ge and 77m Ge production by neutron capture on 76 Ge. To account for full 77m Ge production the cross section used in the simulation was increased by 68% compared to the plain ENDF-based one. Middle: ratio of σ m to total σ d + σ m cross section. An estimate of (50 ± 10)% was used in the analysis. The error bars are used to indicate the range of continuous neutron energies. Right: muon induced 77(m) Ge production rate over neutron energy and time. The Monte Carlo realization corresponds to 1544 kg·year of Gerda Phase II exposure tag events with 77(m) Ge production by prompt coincidences (multiplicity ≥ 1) between muon veto and germanium array is (85 ± 2)%. General muon events show this signature with a rate of 1 × 10 −4 s −1 . This allows to suppress the 77m Ge background by implementing a delayed coincidence cut that removes several 77m Ge half-lives of data after a prompt tagging signal. A dead-time of 6 min results in a reduction of the 77m Ge background to (3.0 ± 0.7) × 10 −6 cts/(keV·kg·year) at an acceptable life time reduction of < 4%. 8 The number of events featuring a prompt coincidence is larger than the prompt 77(m) Ge production itself. Part of the registered signals originate from other processes triggered by the same incident muon, including accompanying neutron captures in the array surroundings. These sibling captures can be used to improve the tagging efficiency for muon events with accompanying isotope production. 41 Ar constitutes the majority of these sibling isotopes. A significant fraction of it is formed by capture of thermalized neutrons. The timing for its production is shown in Fig. 5. It is predominantly described by a capture time of about 271 µs of thermalized neutrons in LAr. The inset shows the number of 41 Ar siblings for 77(m) Ge events, in some cases up to several hundreds of siblings are formed. Their production significantly contributes to prompt and especially delayed signals seen in the germanium array. (60 ± 7)% of 77(m) Ge events not showing the prompt signature still exhibit a germanium signal at > 10 µs. Figure 5 shows the single event multiplicity of these delayed events. This delayed coincidence can be used 8 The efficiency of the Gerda muon veto system is (99.2 +0. 3 −0.4 )% [40].
as further signature to tag muon events with accompanying isotope production. Again the implementation of 6 min dead-time after a delayed tagging coincidence allows to further reduce the 77m Ge background to (1.2 ± 0.5) × 10 −6 cts/(keV·kg·year) with negligible life time reduction. 9 The sequence of processes producing prompt and delayed coincidences between muon veto and germanium detectors is depicted in Fig. 6. In many cases the prompt signal in the germanium detectors is supported by the neutron capture on 76 Ge itself, while for the delayed tagging capture of thermalized neutrons in the surrounding LAr is essential. A systematically underestimated isotope production rate by muon induced neutrons as discussed in Sect. 2.1 could partly compensate. Larger production rates would manifest in an increased chance to tag 77(m) Ge events. Additional reduction could be achieved by facilitating the LAr instrumentation to increase the efficiency to detect muon events with accompanying isotope production by observation of sibling captures. Due to the much longer life-time delayed coincidence cuts will almost not affect the background by ground state 77 Ge. The combined 77(m) Ge background after cuts is (2.7±0.3)×10 −6 cts/(keV·kg·year). However, any improvement in active background suppression based on prompt coincidences like PSD and LAr veto will result in a reduction of the 77 Ge contribution to this number.

Other muon induced backgrounds
Other radioisotopes formed in cosmic muon interactions have only a minor contribution to the background in the search for 0νββ decay of 76 Ge. Different backgrounds due to internal and external occurring subsequent decays were studied in [2]. Only sources exceeding 10 −6 cts/(keV·kg·year) were reported. Simple decay scheme considerations allow to draw qualitative predictions concerning a further suppression of these backgrounds by the Gerda active background rejection strategy and the proposed delayed coincidence cuts. Internal decays of the Ga isotopes 74 Ga and 76 Ga will face a strong suppression from coincident γ 's of more than 500 keV released in their β-decays [41,42]. 10 Due to its non-negligible ground state β transition probability 75 Ga will exhibit only marginal suppression. Nevertheless, the short half-lifes of both 75 Ga of 126 s and 76 Ga of 33 s allow reduction by delayed coincidence. Background originating from 68 Ge/ 68 Ga and 69 Ge electron capture/β + decays will be suppressed by coincidences in the surrounding LAr or other HPGe detectors [44,45]. β-decays of Ar and Cl isotopes in the surrounding LAr are negligible compared to contributions by naturally present background from e.g. 42 K decays [46]. The high energy γ 's from 38 Cl and 40 Cl decays will be largely suppressed by the coincident energy deposit of the initial β in the LAr [47,48].
The prompt muon induced background for the Gerda experiment has been studied in [2,40]. In addition to the muon veto, the active background rejection by AC, LAr veto and PSD further reduces this background.

Conclusions and prospects for future experiments
Distinct features in the production and the decay of radioactive isotopes from cosmic muon interactions allow for a strong reduction of these backgrounds in experiments exploiting an active background rejection strategy. The initial 77(m) Ge background is (4.0 ± 0.4) × 10 −5 cts/(keV·kg·year). State-of-the-art active background rejection techniques in combination with a simple delayed coincidence cut based on tagging muon events with accompanying isotope production by prompt and delayed coincidences between muon veto and germanium array will allow a reduction by more than one order of magnitude to (2.7 ± 0.3)×10 −6 cts/(keV·kg·year) at an acceptable life-time loss of < 4%. The systematic uncertainty on this number is 35 % related to the muon induced isotope production in Geant4. The reduction obtained by the proposed strategy is based on conservative parameters for germanium detector and LAr scintillation light read-out. It amounts to a reduction in muon flux of more than one order of magnitude, which is usually provided by deeper underground laboratories. Taking the equivalent vertical depth definition of [1] and attributing the reduction linearly to a decrease in muon flux, this corresponds to a Gran Sasso depth exceeding 5000 m.w.e. for 77(m) Ge.
In a first stage the next generation experiment Legend will operate about 200 kg of enriched germanium detectors in the Gerda infrastructure at Lngs [4]. Similar or better background rejection capabilities will result in a background contribution comparable to the one described in this paper. This is well below the background goal of the Legend-200 phase at about 10 −4 cts/(keV·kg·year). With a design exposure of about 1 ton·year for Legend-200 will give the unique opportunity to determine the muon induced 77(m) Ge production in-situ at Lngs and thereby verify the predicted rate of 0.21 nuclei/(kg·year).
For the following Legend-1k phase a new facility holding up to 1 ton of HPGe detectors is conceived. Already the 77(m) Ge background obtained for the Gerda setup, exploiting the current active background rejection techniques and a simple delayed coincidence cut, is below the aspired background index goal of about 10 −5 cts/(keV·kg·year). Further reduction can be achieved provided that rigorous measures are taken during the design stage by geometry optimization and material selection with respect to neutron production and propagation.
The possibilities to actively reduce the muon induced background described in this paper equals a virtual increase in Lngs depth and opens the way for next generation experiments with ultra low background requirements.