First results of the NEXT-100 detector using $^{83m}$Kr decays

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Main Authors: 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.
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Published: 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