First results of the NEXT-100 detector using $^{83m}$Kr decays
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arXiv
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| Format: | Preprint |
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2025
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| author | NEXT Collaboration Martínez-Lema, G. Carrete, C. Hervés Torelli, S. Laso, M. Cid Cabaleiro, P. Vázquez Palmeiro, B. Morata, J. A. Hernando Gómez-Cadenas, J. J. Adams, C. Almazán, H. Álvarez, V. Aranburu, A. I. Arazi, L. Arnquist, I. J. Auria-Luna, F. Ayet, S. Ayyad, Y. Azevedo, C. D. R. Bailey, K. Ballester, F. Barcelon, J. E. del Barrio-Torregrosa, M. Bayo, A. Benlloch-Rodríguez, J. M. Borges, F. I. G. M. Brodoline, A. Byrnes, N. Castillo, A. Church, E. Cid, L. Cid, X. Conde, C. A. N. Cortes-Parra, C. Cossío, F. P. Coupe, R. Dey, E. Dietz, P. Echeverria, C. Elorza, M. Esteve, R. Felkai, R. Fernandes, L. M. P. Ferrario, P. Foss, F. W. Freixa, Z. García-Barrena, J. Grocott, J. W. R. Guenette, R. Hauptman, J. Henriques, C. A. O. Herrero-Gómez, P. Herrero, V. Ifergan, Y. Isabel, A. F. B. Jones, B. J. P. Kellerer, F. Larizgoitia, L. Larumbe, A. Lebrun, P. Lopez, F. López-March, N. Madigan, R. Mano, R. D. P. Marauri, A. Marques, A. P. Martín-Albo, J. Martínez, A. Martínez-Vara, M. Miller, R. L. Mistry, K. Molina-Canteras, J. Monrabal, F. Monteiro, C. M. B. Mora, F. J. Navarro, K. E. Novella, P. Nygren, D. R. Oblak, E. Palacio, J. Para, A. Parmaksiz, I. Pazos, A. Pelegrin, J. Maneiro, M. Pérez Querol, M. Renner, J. Rivilla, I. Rogero, C. Rogers, L. Romeo, B. Romo-Luque, C. Ruiz-Chóliz, E. Saharia, P. Santos, F. P. Santos, J. M. F. dos Seemann, M. Shomroni, I. Silva, A. L. M. Silva, P. A. O. C. Simón, A. Soleti, S. R. Sorel, M. Soto-Oton, J. Teixeira, J. M. R. Teruel-Pardo, S. Toledo, J. F. Tonnelé, C. Torrent, J. Trettin, A. Valle, P. R. G. Vanga, M. Veloso, J. F. C. A. Villamil, J. D. Waiton, J. Yubero-Navarro, A. |
| author_facet | NEXT Collaboration Martínez-Lema, G. Carrete, C. Hervés Torelli, S. Laso, M. Cid Cabaleiro, P. Vázquez Palmeiro, B. Morata, J. A. Hernando Gómez-Cadenas, J. J. Adams, C. Almazán, H. Álvarez, V. Aranburu, A. I. Arazi, L. Arnquist, I. J. Auria-Luna, F. Ayet, S. Ayyad, Y. Azevedo, C. D. R. Bailey, K. Ballester, F. Barcelon, J. E. del Barrio-Torregrosa, M. Bayo, A. Benlloch-Rodríguez, J. M. Borges, F. I. G. M. Brodoline, A. Byrnes, N. Castillo, A. Church, E. Cid, L. Cid, X. Conde, C. A. N. Cortes-Parra, C. Cossío, F. P. Coupe, R. Dey, E. Dietz, P. Echeverria, C. Elorza, M. Esteve, R. Felkai, R. Fernandes, L. M. P. Ferrario, P. Foss, F. W. Freixa, Z. García-Barrena, J. Grocott, J. W. R. Guenette, R. Hauptman, J. Henriques, C. A. O. Herrero-Gómez, P. Herrero, V. Ifergan, Y. Isabel, A. F. B. Jones, B. J. P. Kellerer, F. Larizgoitia, L. Larumbe, A. Lebrun, P. Lopez, F. López-March, N. Madigan, R. Mano, R. D. P. Marauri, A. Marques, A. P. Martín-Albo, J. Martínez, A. Martínez-Vara, M. Miller, R. L. Mistry, K. Molina-Canteras, J. Monrabal, F. Monteiro, C. M. B. Mora, F. J. Navarro, K. E. Novella, P. Nygren, D. R. Oblak, E. Palacio, J. Para, A. Parmaksiz, I. Pazos, A. Pelegrin, J. Maneiro, M. Pérez Querol, M. Renner, J. Rivilla, I. Rogero, C. Rogers, L. Romeo, B. Romo-Luque, C. Ruiz-Chóliz, E. Saharia, P. Santos, F. P. Santos, J. M. F. dos Seemann, M. Shomroni, I. Silva, A. L. M. Silva, P. A. O. C. Simón, A. Soleti, S. R. Sorel, M. Soto-Oton, J. Teixeira, J. M. R. Teruel-Pardo, S. Toledo, J. F. Tonnelé, C. Torrent, J. Trettin, A. Valle, P. R. G. Vanga, M. Veloso, J. F. C. A. Villamil, J. D. Waiton, J. Yubero-Navarro, A. |
| contents | The NEXT collaboration is investigating the double beta decay of $^{136}$Xe using high-pressure gas electroluminescent time projection chambers, which provide excellent energy resolution together with a robust topological signature. Operating at the Laboratorio Subterráneo de Canfranc (LSC) and building on the success of the NEXT-White detector, the NEXT-100 apparatus began commissioning in May 2024 and started operation with xenon at a pressure of 4 bar in October 2024.
We report here the first results obtained with NEXT-100 using low-energy calibration data from $^{83m}$Kr decays, which allow mapping of the detector response in the active volume and monitoring of its stability over time. After homogenizing the light response, we achieve an energy resolution of 4.37% FWHM at 41.5 keV for $^{83m}$Kr point-like energy deposits contained in a radius of 425 mm. In a fiducial region representing the operating conditions of NEXT-100 at 10 bar we obtain an improved energy resolution of 4.16% FWHM. These results are in good agreement with that obtained in NEXT-White, and an $E^{-1/2}$ extrapolation to $Q_{ββ}$ yields an energy resolution close to 0.5% FWHM, well below the 1% FWHM design target. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2511_01710 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | First results of the NEXT-100 detector using $^{83m}$Kr decays NEXT Collaboration Martínez-Lema, G. Carrete, C. Hervés Torelli, S. Laso, M. Cid Cabaleiro, P. Vázquez Palmeiro, B. Morata, J. A. Hernando Gómez-Cadenas, J. J. Adams, C. Almazán, H. Álvarez, V. Aranburu, A. I. Arazi, L. Arnquist, I. J. Auria-Luna, F. Ayet, S. Ayyad, Y. Azevedo, C. D. R. Bailey, K. Ballester, F. Barcelon, J. E. del Barrio-Torregrosa, M. Bayo, A. Benlloch-Rodríguez, J. M. Borges, F. I. G. M. Brodoline, A. Byrnes, N. Castillo, A. Church, E. Cid, L. Cid, X. Conde, C. A. N. Cortes-Parra, C. Cossío, F. P. Coupe, R. Dey, E. Dietz, P. Echeverria, C. Elorza, M. Esteve, R. Felkai, R. Fernandes, L. M. P. Ferrario, P. Foss, F. W. Freixa, Z. García-Barrena, J. Grocott, J. W. R. Guenette, R. Hauptman, J. Henriques, C. A. O. Herrero-Gómez, P. Herrero, V. Ifergan, Y. Isabel, A. F. B. Jones, B. J. P. Kellerer, F. Larizgoitia, L. Larumbe, A. Lebrun, P. Lopez, F. López-March, N. Madigan, R. Mano, R. D. P. Marauri, A. Marques, A. P. Martín-Albo, J. Martínez, A. Martínez-Vara, M. Miller, R. L. Mistry, K. Molina-Canteras, J. Monrabal, F. Monteiro, C. M. B. Mora, F. J. Navarro, K. E. Novella, P. Nygren, D. R. Oblak, E. Palacio, J. Para, A. Parmaksiz, I. Pazos, A. Pelegrin, J. Maneiro, M. Pérez Querol, M. Renner, J. Rivilla, I. Rogero, C. Rogers, L. Romeo, B. Romo-Luque, C. Ruiz-Chóliz, E. Saharia, P. Santos, F. P. Santos, J. M. F. dos Seemann, M. Shomroni, I. Silva, A. L. M. Silva, P. A. O. C. Simón, A. Soleti, S. R. Sorel, M. Soto-Oton, J. Teixeira, J. M. R. Teruel-Pardo, S. Toledo, J. F. Tonnelé, C. Torrent, J. Trettin, A. Valle, P. R. G. Vanga, M. Veloso, J. F. C. A. Villamil, J. D. Waiton, J. Yubero-Navarro, A. High Energy Physics - Experiment Instrumentation and Detectors The NEXT collaboration is investigating the double beta decay of $^{136}$Xe using high-pressure gas electroluminescent time projection chambers, which provide excellent energy resolution together with a robust topological signature. Operating at the Laboratorio Subterráneo de Canfranc (LSC) and building on the success of the NEXT-White detector, the NEXT-100 apparatus began commissioning in May 2024 and started operation with xenon at a pressure of 4 bar in October 2024. We report here the first results obtained with NEXT-100 using low-energy calibration data from $^{83m}$Kr decays, which allow mapping of the detector response in the active volume and monitoring of its stability over time. After homogenizing the light response, we achieve an energy resolution of 4.37% FWHM at 41.5 keV for $^{83m}$Kr point-like energy deposits contained in a radius of 425 mm. In a fiducial region representing the operating conditions of NEXT-100 at 10 bar we obtain an improved energy resolution of 4.16% FWHM. These results are in good agreement with that obtained in NEXT-White, and an $E^{-1/2}$ extrapolation to $Q_{ββ}$ yields an energy resolution close to 0.5% FWHM, well below the 1% FWHM design target. |
| title | First results of the NEXT-100 detector using $^{83m}$Kr decays |
| topic | High Energy Physics - Experiment Instrumentation and Detectors |
| url | https://arxiv.org/abs/2511.01710 |