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description Publicationkeyboard_double_arrow_right Article , Preprint 2024Embargo end date: 01 Jan 2024 Italy, France, France, United States, Italy, France, ItalyPublisher:American Physical Society (APS) Funded by:NSF | CUORE: Phase-I Constructi..., NSF | CUORE and MAJORANA:Next G..., NSF | RUI: A Program of Undergr... +6 projectsNSF| CUORE: Phase-I Construction and Crystal Bolometer Research and Development ,NSF| CUORE and MAJORANA:Next Generation Neutrino-Less Double-Beta Experiments ,NSF| RUI: A Program of Undergraduate Participation in the Search for Rare Events with CUORE ,NSF| Next Generation Double-Beta Experimints:CUORE/CUORICINO and Majorana ,NSF| UCLA CUORE Neutrino Physics Research Program ,NSF| RUI: Analysis, Simulation, and Onsite Activities Contributing to the Search for Neutrinoless Double Beta Decay in Tellurium Using the CUORE Detector ,NSF| Participation in the Construction and Operation of the CUORE and Majorana Neutrinoless Double-Beta Decay Experiments ,NSF| Searches for Neutrinoless Double Beta Decay with Bolometric Detectors ,NSF| Searches for Neutrinoless Double Beta Decay with Bolometric DetectorsCUORE Collaboration; Adams, D. Q.; Alduino, C.; Alfonso, K.; Avignone, F. T.; Azzolini, O.; Bari, G.; Bellini, F.; Benato, G.; Beretta, M.; Biassoni, M.; Branca, A.; Brofferio, C.; Bucci, C.; Camilleri, J.; Caminata, A.; Campani, A.; Cao, J.; Capelli, S.; Capelli, C.; Cappelli, L.; Cardani, L.; Carniti, P.; Casali, N.; Celi, E.; Chiesa, D.; Clemenza, M.; Cremonesi, O.; Creswick, R. J.; D'Addabbo, A.; Dafinei, I.; Del Corso, F.; Dell'Oro, S.; Di Domizio, S.; Di Lorenzo, S.; Dixon, T.; Dompè, V.; Fang, D. Q.; Fantini, G.; Faverzani, M.; Ferri, E.; Ferroni, F.; Fiorini, E.; Franceschi, M. A.; Freedman, S. J.; Fu, S. H.; Fujikawa, B. K.; Ghislandi, S.; Giachero, A.; Girola, M.; Gironi, L.; Giuliani, A.; Gorla, P.; Gotti, C.; Guillaumon, P. V.; Gutierrez, T. D.; Han, K.; Hansen, E. V.; Heeger, K. M.; Helis, D. L.; Huang, H. Z.; Keppel, G.; Kolomensky, Yu. G.; Kowalski, R.; Liu, R.; Ma, L.; Ma, Y. G.; Marini, L.; Maruyama, R. H.; Mayer, D.; Mei, Y.; Moore, M. N.; Napolitano, T.; Nastasi, M.; Nones, C.; Norman, E. B.; Nucciotti, A.; Nutini, I.; O'Donnell, T.; Olmi, M.; Oregui, B. T.; Ouellet, J. L.; Pagan, S.; Pagliarone, C. E.; Pagnanini, L.; Pallavicini, M.; Pattavina, L.; Pavan, M.; Pessina, G.; Pettinacci, V.; Pira, C.; Pirro, S.; Ponce, I.; Pottebaum, E. G.; Pozzi, S.; Previtali, E.; Puiu, A.; Quitadamo, S.; Ressa, A.; Rosenfeld, C.; Schmidt, B.; Sharma, V.; Singh, V.; Sisti, M.; Speller, D.; Surukuchi, P. T.; Taffarello, L.; Tomei, C.; Torres, J. A; Vetter, K. J.; Vignati, M.; Wagaarachchi, S. L.; Welliver, B.; Wilson, J.; Wilson, K.; Winslow, L. A.; Zimmermann, S.; Zucchelli, S.;handle: 10281/525257 , 11573/1720701 , 11567/1223778
We present the model we developed to reconstruct the CUORE radioactive background based on the analysis of an experimental exposure of 1038.4 kg yr. The data reconstruction relies on a simultaneous Bayesian fit applied to energy spectra over a broad energy range. The high granularity of the CUORE detector, together with the large exposure and extended stable operations, allow for an in-depth exploration of both spatial and time dependence of backgrounds. We achieve high sensitivity to both bulk and surface activities of the materials of the setup, detecting levels as low as 10 nBq kg$^{-1}$ and 0.1 nBq cm$^{-2}$, respectively. We compare the contamination levels we extract from the background model with prior radio-assay data, which informs future background risk mitigation strategies. The results of this background model play a crucial role in constructing the background budget for the CUPID experiment as it will exploit the same CUORE infrastructure.
Archivio della ricer... arrow_drop_down University of California: eScholarshipArticle . 2024Full-Text: https://escholarship.org/uc/item/9370z9c3Data sources: Bielefeld Academic Search Engine (BASE)https://doi.org/10.1103/physre...Article . 2024 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: CrossrefeScholarship - University of CaliforniaArticle . 2024Data sources: eScholarship - University of Californiaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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more_vert Archivio della ricer... arrow_drop_down University of California: eScholarshipArticle . 2024Full-Text: https://escholarship.org/uc/item/9370z9c3Data sources: Bielefeld Academic Search Engine (BASE)https://doi.org/10.1103/physre...Article . 2024 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: CrossrefeScholarship - University of CaliforniaArticle . 2024Data sources: eScholarship - University of Californiaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2023Embargo end date: 01 Jan 2022 Spain, Finland, France, Italy, Italy, Italy, Finland, Italy, ItalyPublisher:American Physical Society (APS) Funded by:AKA | Theoretical tools for rar..., AKA | Theoretical tools for rar..., EC | LUCIFER +1 projectsAKA| Theoretical tools for rare nuclear decays and dark matter searches ,AKA| Theoretical tools for rare nuclear decays and dark matter searches ,EC| LUCIFER ,AKA| Theoretical tools for rare nuclear decays and dark matter searches0 Collaboration; Azzolini, O.; Beeman, J. W.; Bellini, F.; Beretta, M.; Biassoni, M.; Brofferio, C.; Bucci, C.; Capelli, S.; Caracciolo, V.; Cardani, L.; Carniti, P.; Casali, N.; Celi, E.; Chiesa, D.; Clemenza, M.; Colantoni, I.; Cremonesi, O.; Cruciani, A.; D'Addabbo, A.; Dafinei, I.; Di Domizio, S.; Dompè, V.; Fantini, G.; Ferroni, F.; Gironi, L.; Giuliani, A.; Gorla, P.; Gotti, C.; Keppel, G.; Kotila, J.; Martinez, M.; Nagorny, S.; Nastasi, M.; Nisi, S.; Nones, C.; Orlandi, D.; Pagnanini, L.; Pallavicini, M.; Pattavina, L.; Pavan, M.; Pessina, G.; Pettinacci, V.; Pirro, S.; Pozzi, S.; Previtali, E.; Puiu, A.; Ressa, A.; Rusconi, C.; Schäffner, K.; Tomei, C.; Vignati, M.; Zolotarova, A. S.;handle: 20.500.14243/464980 , 10281/409996 , 2108/315861 , 11573/1671725 , 11567/1159765
We present the first search for the Majoron-emitting modes of the neutrinoless double $β$ decay ($0νββχ_0$) using scintillating cryogenic calorimeters. We analysed the CUPID-0 Phase I data using a Bayesian approach to reconstruct the background sources activities, and evaluate the potential contribution of the $^{82}$Se $0νββχ_0$. We considered several possible theoretical models which predict the existence of a Majoron-like boson coupling to the neutrino. The energy spectra arising from the emission of such bosons in the neutrinoless double $β$ decay have spectral indices $n=$ 1, 2, 3 or 7. We found no evidence of any of these decay modes, setting a lower limit (90% of credibility interval) on the half-life of 1.2 $\times$ 10$^{23}$ yr in the case of $n=$ 1, 3.8 $\times$ 10$^{22}$ yr for $n=$ 2, 1.4 $\times$ 10$^{22}$ yr for $n=$ 3 and 2.2 $\times$ 10$^{21}$ yr for $n=$ 7. These are the best limits on the $0νββχ_0$ half-life of the $^{82}$Se, and demonstrate the potentiality of the CUPID-0 technology in this field.
BOA - Bicocca Open A... arrow_drop_down Archivio della ricerca- Università di Roma La SapienzaArticle . 2023License: CC BYData sources: Archivio della ricerca- Università di Roma La SapienzaDigital Repository of University of Zaragoza (ZAGUAN)Article . 2023License: CC BYFull-Text: http://zaguan.unizar.es/record/125809Data sources: Bielefeld Academic Search Engine (BASE)https://doi.org/10.1103/physre...Article . 2023 . Peer-reviewedLicense: CC BYData sources: CrossrefRecolector de Ciencia Abierta, RECOLECTAArticle . 2023License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAJyväskylä University Digital ArchiveArticle . 2023 . Peer-reviewedData sources: Jyväskylä University Digital ArchiveDigital Repository of University of ZaragozaArticle . 2023License: CC BYData sources: Digital Repository of University of ZaragozaArchivio della Ricerca - Università di Roma Tor vergataArticle . 2023Data sources: Archivio della Ricerca - Università di Roma Tor vergatahttps://dx.doi.org/10.48550/ar...Article . 2022License: arXiv Non-Exclusive DistributionData sources: DataciteArchivio della Ricerca - Università di Roma Tor vergataArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu6 citations 6 popularity Top 10% influence Average impulse Top 10% Powered by BIP!
more_vert BOA - Bicocca Open A... arrow_drop_down Archivio della ricerca- Università di Roma La SapienzaArticle . 2023License: CC BYData sources: Archivio della ricerca- Università di Roma La SapienzaDigital Repository of University of Zaragoza (ZAGUAN)Article . 2023License: CC BYFull-Text: http://zaguan.unizar.es/record/125809Data sources: Bielefeld Academic Search Engine (BASE)https://doi.org/10.1103/physre...Article . 2023 . Peer-reviewedLicense: CC BYData sources: CrossrefRecolector de Ciencia Abierta, RECOLECTAArticle . 2023License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAJyväskylä University Digital ArchiveArticle . 2023 . Peer-reviewedData sources: Jyväskylä University Digital ArchiveDigital Repository of University of ZaragozaArticle . 2023License: CC BYData sources: Digital Repository of University of ZaragozaArchivio della Ricerca - Università di Roma Tor vergataArticle . 2023Data sources: Archivio della Ricerca - Università di Roma Tor vergatahttps://dx.doi.org/10.48550/ar...Article . 2022License: arXiv Non-Exclusive DistributionData sources: DataciteArchivio della Ricerca - Università di Roma Tor vergataArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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description Publicationkeyboard_double_arrow_right Article , Preprint 2024Embargo end date: 01 Jan 2024 Italy, France, France, United States, Italy, France, ItalyPublisher:American Physical Society (APS) Funded by:NSF | CUORE: Phase-I Constructi..., NSF | CUORE and MAJORANA:Next G..., NSF | RUI: A Program of Undergr... +6 projectsNSF| CUORE: Phase-I Construction and Crystal Bolometer Research and Development ,NSF| CUORE and MAJORANA:Next Generation Neutrino-Less Double-Beta Experiments ,NSF| RUI: A Program of Undergraduate Participation in the Search for Rare Events with CUORE ,NSF| Next Generation Double-Beta Experimints:CUORE/CUORICINO and Majorana ,NSF| UCLA CUORE Neutrino Physics Research Program ,NSF| RUI: Analysis, Simulation, and Onsite Activities Contributing to the Search for Neutrinoless Double Beta Decay in Tellurium Using the CUORE Detector ,NSF| Participation in the Construction and Operation of the CUORE and Majorana Neutrinoless Double-Beta Decay Experiments ,NSF| Searches for Neutrinoless Double Beta Decay with Bolometric Detectors ,NSF| Searches for Neutrinoless Double Beta Decay with Bolometric DetectorsCUORE Collaboration; Adams, D. Q.; Alduino, C.; Alfonso, K.; Avignone, F. T.; Azzolini, O.; Bari, G.; Bellini, F.; Benato, G.; Beretta, M.; Biassoni, M.; Branca, A.; Brofferio, C.; Bucci, C.; Camilleri, J.; Caminata, A.; Campani, A.; Cao, J.; Capelli, S.; Capelli, C.; Cappelli, L.; Cardani, L.; Carniti, P.; Casali, N.; Celi, E.; Chiesa, D.; Clemenza, M.; Cremonesi, O.; Creswick, R. J.; D'Addabbo, A.; Dafinei, I.; Del Corso, F.; Dell'Oro, S.; Di Domizio, S.; Di Lorenzo, S.; Dixon, T.; Dompè, V.; Fang, D. Q.; Fantini, G.; Faverzani, M.; Ferri, E.; Ferroni, F.; Fiorini, E.; Franceschi, M. A.; Freedman, S. J.; Fu, S. H.; Fujikawa, B. K.; Ghislandi, S.; Giachero, A.; Girola, M.; Gironi, L.; Giuliani, A.; Gorla, P.; Gotti, C.; Guillaumon, P. V.; Gutierrez, T. D.; Han, K.; Hansen, E. V.; Heeger, K. M.; Helis, D. L.; Huang, H. Z.; Keppel, G.; Kolomensky, Yu. G.; Kowalski, R.; Liu, R.; Ma, L.; Ma, Y. G.; Marini, L.; Maruyama, R. H.; Mayer, D.; Mei, Y.; Moore, M. N.; Napolitano, T.; Nastasi, M.; Nones, C.; Norman, E. B.; Nucciotti, A.; Nutini, I.; O'Donnell, T.; Olmi, M.; Oregui, B. T.; Ouellet, J. L.; Pagan, S.; Pagliarone, C. E.; Pagnanini, L.; Pallavicini, M.; Pattavina, L.; Pavan, M.; Pessina, G.; Pettinacci, V.; Pira, C.; Pirro, S.; Ponce, I.; Pottebaum, E. G.; Pozzi, S.; Previtali, E.; Puiu, A.; Quitadamo, S.; Ressa, A.; Rosenfeld, C.; Schmidt, B.; Sharma, V.; Singh, V.; Sisti, M.; Speller, D.; Surukuchi, P. T.; Taffarello, L.; Tomei, C.; Torres, J. A; Vetter, K. J.; Vignati, M.; Wagaarachchi, S. L.; Welliver, B.; Wilson, J.; Wilson, K.; Winslow, L. A.; Zimmermann, S.; Zucchelli, S.;handle: 10281/525257 , 11573/1720701 , 11567/1223778
We present the model we developed to reconstruct the CUORE radioactive background based on the analysis of an experimental exposure of 1038.4 kg yr. The data reconstruction relies on a simultaneous Bayesian fit applied to energy spectra over a broad energy range. The high granularity of the CUORE detector, together with the large exposure and extended stable operations, allow for an in-depth exploration of both spatial and time dependence of backgrounds. We achieve high sensitivity to both bulk and surface activities of the materials of the setup, detecting levels as low as 10 nBq kg$^{-1}$ and 0.1 nBq cm$^{-2}$, respectively. We compare the contamination levels we extract from the background model with prior radio-assay data, which informs future background risk mitigation strategies. The results of this background model play a crucial role in constructing the background budget for the CUPID experiment as it will exploit the same CUORE infrastructure.
Archivio della ricer... arrow_drop_down University of California: eScholarshipArticle . 2024Full-Text: https://escholarship.org/uc/item/9370z9c3Data sources: Bielefeld Academic Search Engine (BASE)https://doi.org/10.1103/physre...Article . 2024 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: CrossrefeScholarship - University of CaliforniaArticle . 2024Data sources: eScholarship - University of Californiaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.110.052003&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
more_vert Archivio della ricer... arrow_drop_down University of California: eScholarshipArticle . 2024Full-Text: https://escholarship.org/uc/item/9370z9c3Data sources: Bielefeld Academic Search Engine (BASE)https://doi.org/10.1103/physre...Article . 2024 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: CrossrefeScholarship - University of CaliforniaArticle . 2024Data sources: eScholarship - University of Californiaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.110.052003&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2023Embargo end date: 01 Jan 2022 Spain, Finland, France, Italy, Italy, Italy, Finland, Italy, ItalyPublisher:American Physical Society (APS) Funded by:AKA | Theoretical tools for rar..., AKA | Theoretical tools for rar..., EC | LUCIFER +1 projectsAKA| Theoretical tools for rare nuclear decays and dark matter searches ,AKA| Theoretical tools for rare nuclear decays and dark matter searches ,EC| LUCIFER ,AKA| Theoretical tools for rare nuclear decays and dark matter searches0 Collaboration; Azzolini, O.; Beeman, J. W.; Bellini, F.; Beretta, M.; Biassoni, M.; Brofferio, C.; Bucci, C.; Capelli, S.; Caracciolo, V.; Cardani, L.; Carniti, P.; Casali, N.; Celi, E.; Chiesa, D.; Clemenza, M.; Colantoni, I.; Cremonesi, O.; Cruciani, A.; D'Addabbo, A.; Dafinei, I.; Di Domizio, S.; Dompè, V.; Fantini, G.; Ferroni, F.; Gironi, L.; Giuliani, A.; Gorla, P.; Gotti, C.; Keppel, G.; Kotila, J.; Martinez, M.; Nagorny, S.; Nastasi, M.; Nisi, S.; Nones, C.; Orlandi, D.; Pagnanini, L.; Pallavicini, M.; Pattavina, L.; Pavan, M.; Pessina, G.; Pettinacci, V.; Pirro, S.; Pozzi, S.; Previtali, E.; Puiu, A.; Ressa, A.; Rusconi, C.; Schäffner, K.; Tomei, C.; Vignati, M.; Zolotarova, A. S.;handle: 20.500.14243/464980 , 10281/409996 , 2108/315861 , 11573/1671725 , 11567/1159765
We present the first search for the Majoron-emitting modes of the neutrinoless double $β$ decay ($0νββχ_0$) using scintillating cryogenic calorimeters. We analysed the CUPID-0 Phase I data using a Bayesian approach to reconstruct the background sources activities, and evaluate the potential contribution of the $^{82}$Se $0νββχ_0$. We considered several possible theoretical models which predict the existence of a Majoron-like boson coupling to the neutrino. The energy spectra arising from the emission of such bosons in the neutrinoless double $β$ decay have spectral indices $n=$ 1, 2, 3 or 7. We found no evidence of any of these decay modes, setting a lower limit (90% of credibility interval) on the half-life of 1.2 $\times$ 10$^{23}$ yr in the case of $n=$ 1, 3.8 $\times$ 10$^{22}$ yr for $n=$ 2, 1.4 $\times$ 10$^{22}$ yr for $n=$ 3 and 2.2 $\times$ 10$^{21}$ yr for $n=$ 7. These are the best limits on the $0νββχ_0$ half-life of the $^{82}$Se, and demonstrate the potentiality of the CUPID-0 technology in this field.
BOA - Bicocca Open A... arrow_drop_down Archivio della ricerca- Università di Roma La SapienzaArticle . 2023License: CC BYData sources: Archivio della ricerca- Università di Roma La SapienzaDigital Repository of University of Zaragoza (ZAGUAN)Article . 2023License: CC BYFull-Text: http://zaguan.unizar.es/record/125809Data sources: Bielefeld Academic Search Engine (BASE)https://doi.org/10.1103/physre...Article . 2023 . Peer-reviewedLicense: CC BYData sources: CrossrefRecolector de Ciencia Abierta, RECOLECTAArticle . 2023License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAJyväskylä University Digital ArchiveArticle . 2023 . Peer-reviewedData sources: Jyväskylä University Digital ArchiveDigital Repository of University of ZaragozaArticle . 2023License: CC BYData sources: Digital Repository of University of ZaragozaArchivio della Ricerca - Università di Roma Tor vergataArticle . 2023Data sources: Archivio della Ricerca - Università di Roma Tor vergatahttps://dx.doi.org/10.48550/ar...Article . 2022License: arXiv Non-Exclusive DistributionData sources: DataciteArchivio della Ricerca - Università di Roma Tor vergataArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu6 citations 6 popularity Top 10% influence Average impulse Top 10% Powered by BIP!
more_vert BOA - Bicocca Open A... arrow_drop_down Archivio della ricerca- Università di Roma La SapienzaArticle . 2023License: CC BYData sources: Archivio della ricerca- Università di Roma La SapienzaDigital Repository of University of Zaragoza (ZAGUAN)Article . 2023License: CC BYFull-Text: http://zaguan.unizar.es/record/125809Data sources: Bielefeld Academic Search Engine (BASE)https://doi.org/10.1103/physre...Article . 2023 . Peer-reviewedLicense: CC BYData sources: CrossrefRecolector de Ciencia Abierta, RECOLECTAArticle . 2023License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAJyväskylä University Digital ArchiveArticle . 2023 . Peer-reviewedData sources: Jyväskylä University Digital ArchiveDigital Repository of University of ZaragozaArticle . 2023License: CC BYData sources: Digital Repository of University of ZaragozaArchivio della Ricerca - Università di Roma Tor vergataArticle . 2023Data sources: Archivio della Ricerca - Università di Roma Tor vergatahttps://dx.doi.org/10.48550/ar...Article . 2022License: arXiv Non-Exclusive DistributionData sources: DataciteArchivio della Ricerca - Università di Roma Tor vergataArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.107.032006&type=result"></script>'); --> </script>
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