Image de couverture de livre

Demonstration of Event Position Reconstruction based on Diffusion in the NEXT-White Detector

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Haefner, J., Navarro, K. E., Guenette, R., Jones, B. J. P., Tripathi, A., Adams, C., Almazán, H., Álvarez, V., Aparicio, B., Aranburu, A. I., Arazi, L., Arnquist, I. J., Auria-Luna, F., Ayet, S., Azevedo, C. D. R., Bailey, K., Ballester, F., del Barrio-Torregrosa, M., Bayo, A., BenllochRodríguez, J. M., Borges, F. I. G. M., Brodolin, A., Byrnes, N., Cárcel, S., Carrión, J. V., Cebrián, S., Church, E., Cid, L., Conde, C. A. N., Contreras, T., Cossío, F. P., Dey, E., Díaz, G., Dickel, T., Elorza, M., Escada, J., Esteve, R., Felkai, R., Fernandes, L. M. P., Ferrario, P., Ferreira, A. L., Foss, F. W., Freitas, E. D. C., Freixa, Z., Generowicz, J., Goldschmidt, A., Gómez-Cadenas, J. J., González, R., Grocott, J., Hafidi, K., Hauptman, J., Henriques, C. A. O., Morata, J. A. Hernando, Herrero-Gómez, P., Herrero, V., Carrete, C. Hervés, Ifergan, Y., Labarga, L., Larizgoitia, L., Larumbe, A., Lebrun, P., Lopez, F., López-March, N., Madigan, R., Mano, R. D. P., Marques, A. P., Martín-Albo, J., Martínez-Lema, G., Martínez-Vara, M., Meziani, Z. E., Miller, R. L., Mistry, K., Molina-Canteras, J., Monrabal, F., Monteiro, C. M. B., Mora, F. J., Vidal, J. Muñoz, Novella, P., Nuñez, A., Nygren, D. R., Oblak, E., Palacio, J., Palmeiro, B., Para, A., Parmaksiz, I., Pelegrin, J., Maneiro, M. Pérez, Querol, M., Redwine, A. B., Renner, J., Rivilla, I., Rodríguez, J., Rogero, C., Rogers, L., Romeo, B., Romo-Luque, C., Santos, F. P., Santos, J. M. F. dos, Shomroni, I., Simón, A., Soleti, S. R., Sorel, M., Soto-Oton, J., Teixeira, J. M. R., Toledo, J. F., Torrent, J., Trettin, A., Usón, A., Veloso, J. F. C. A., Waiton, J., White, J. T.
Format:	Preprint
Publié:	2023
Sujets:	High Energy Physics - Experiment Instrumentation and Detectors
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

_version_	1866911800050581504
author	Haefner, J. Navarro, K. E. Guenette, R. Jones, B. J. P. Tripathi, A. Adams, C. Almazán, H. Álvarez, V. Aparicio, B. Aranburu, A. I. Arazi, L. Arnquist, I. J. Auria-Luna, F. Ayet, S. Azevedo, C. D. R. Bailey, K. Ballester, F. del Barrio-Torregrosa, M. Bayo, A. BenllochRodríguez, J. M. Borges, F. I. G. M. Brodolin, A. Byrnes, N. Cárcel, S. Carrión, J. V. Cebrián, S. Church, E. Cid, L. Conde, C. A. N. Contreras, T. Cossío, F. P. Dey, E. Díaz, G. Dickel, T. Elorza, M. Escada, J. Esteve, R. Felkai, R. Fernandes, L. M. P. Ferrario, P. Ferreira, A. L. Foss, F. W. Freitas, E. D. C. Freixa, Z. Generowicz, J. Goldschmidt, A. Gómez-Cadenas, J. J. González, R. Grocott, J. Hafidi, K. Hauptman, J. Henriques, C. A. O. Morata, J. A. Hernando Herrero-Gómez, P. Herrero, V. Carrete, C. Hervés Ifergan, Y. Labarga, L. Larizgoitia, L. Larumbe, A. Lebrun, P. Lopez, F. López-March, N. Madigan, R. Mano, R. D. P. Marques, A. P. Martín-Albo, J. Martínez-Lema, G. Martínez-Vara, M. Meziani, Z. E. Miller, R. L. Mistry, K. Molina-Canteras, J. Monrabal, F. Monteiro, C. M. B. Mora, F. J. Vidal, J. Muñoz Novella, P. Nuñez, A. Nygren, D. R. Oblak, E. Palacio, J. Palmeiro, B. Para, A. Parmaksiz, I. Pelegrin, J. Maneiro, M. Pérez Querol, M. Redwine, A. B. Renner, J. Rivilla, I. Rodríguez, J. Rogero, C. Rogers, L. Romeo, B. Romo-Luque, C. Santos, F. P. Santos, J. M. F. dos Shomroni, I. Simón, A. Soleti, S. R. Sorel, M. Soto-Oton, J. Teixeira, J. M. R. Toledo, J. F. Torrent, J. Trettin, A. Usón, A. Veloso, J. F. C. A. Waiton, J. White, J. T.
author_facet	Haefner, J. Navarro, K. E. Guenette, R. Jones, B. J. P. Tripathi, A. Adams, C. Almazán, H. Álvarez, V. Aparicio, B. Aranburu, A. I. Arazi, L. Arnquist, I. J. Auria-Luna, F. Ayet, S. Azevedo, C. D. R. Bailey, K. Ballester, F. del Barrio-Torregrosa, M. Bayo, A. BenllochRodríguez, J. M. Borges, F. I. G. M. Brodolin, A. Byrnes, N. Cárcel, S. Carrión, J. V. Cebrián, S. Church, E. Cid, L. Conde, C. A. N. Contreras, T. Cossío, F. P. Dey, E. Díaz, G. Dickel, T. Elorza, M. Escada, J. Esteve, R. Felkai, R. Fernandes, L. M. P. Ferrario, P. Ferreira, A. L. Foss, F. W. Freitas, E. D. C. Freixa, Z. Generowicz, J. Goldschmidt, A. Gómez-Cadenas, J. J. González, R. Grocott, J. Hafidi, K. Hauptman, J. Henriques, C. A. O. Morata, J. A. Hernando Herrero-Gómez, P. Herrero, V. Carrete, C. Hervés Ifergan, Y. Labarga, L. Larizgoitia, L. Larumbe, A. Lebrun, P. Lopez, F. López-March, N. Madigan, R. Mano, R. D. P. Marques, A. P. Martín-Albo, J. Martínez-Lema, G. Martínez-Vara, M. Meziani, Z. E. Miller, R. L. Mistry, K. Molina-Canteras, J. Monrabal, F. Monteiro, C. M. B. Mora, F. J. Vidal, J. Muñoz Novella, P. Nuñez, A. Nygren, D. R. Oblak, E. Palacio, J. Palmeiro, B. Para, A. Parmaksiz, I. Pelegrin, J. Maneiro, M. Pérez Querol, M. Redwine, A. B. Renner, J. Rivilla, I. Rodríguez, J. Rogero, C. Rogers, L. Romeo, B. Romo-Luque, C. Santos, F. P. Santos, J. M. F. dos Shomroni, I. Simón, A. Soleti, S. R. Sorel, M. Soto-Oton, J. Teixeira, J. M. R. Toledo, J. F. Torrent, J. Trettin, A. Usón, A. Veloso, J. F. C. A. Waiton, J. White, J. T.
contents	Noble element time projection chambers are a leading technology for rare event detection in physics, such as for dark matter and neutrinoless double beta decay searches. Time projection chambers typically assign event position in the drift direction using the relative timing of prompt scintillation and delayed charge collection signals, allowing for reconstruction of an absolute position in the drift direction. In this paper, alternate methods for assigning event drift distance via quantification of electron diffusion in a pure high pressure xenon gas time projection chamber are explored. Data from the NEXT-White detector demonstrate the ability to achieve good position assignment accuracy for both high- and low-energy events. Using point-like energy deposits from $^{83\mathrm{m}}$Kr calibration electron captures ($E\sim45$keV), the position of origin of low-energy events is determined to $2~$cm precision with bias $< 1$mm. A convolutional neural network approach is then used to quantify diffusion for longer tracks (E$\geq$1.5MeV), yielding a precision of 3cm on the event barycenter. The precision achieved with these methods indicates the feasibility energy calibrations of better than 1% FWHM at Q$_{ββ}$ in pure xenon, as well as the potential for event fiducialization in large future detectors using an alternate method that does not rely on primary scintillation.
format	Preprint
id	arxiv_https___arxiv_org_abs_2311_03441
institution	arXiv
publishDate	2023
record_format	arxiv
spellingShingle	Demonstration of Event Position Reconstruction based on Diffusion in the NEXT-White Detector Haefner, J. Navarro, K. E. Guenette, R. Jones, B. J. P. Tripathi, A. Adams, C. Almazán, H. Álvarez, V. Aparicio, B. Aranburu, A. I. Arazi, L. Arnquist, I. J. Auria-Luna, F. Ayet, S. Azevedo, C. D. R. Bailey, K. Ballester, F. del Barrio-Torregrosa, M. Bayo, A. BenllochRodríguez, J. M. Borges, F. I. G. M. Brodolin, A. Byrnes, N. Cárcel, S. Carrión, J. V. Cebrián, S. Church, E. Cid, L. Conde, C. A. N. Contreras, T. Cossío, F. P. Dey, E. Díaz, G. Dickel, T. Elorza, M. Escada, J. Esteve, R. Felkai, R. Fernandes, L. M. P. Ferrario, P. Ferreira, A. L. Foss, F. W. Freitas, E. D. C. Freixa, Z. Generowicz, J. Goldschmidt, A. Gómez-Cadenas, J. J. González, R. Grocott, J. Hafidi, K. Hauptman, J. Henriques, C. A. O. Morata, J. A. Hernando Herrero-Gómez, P. Herrero, V. Carrete, C. Hervés Ifergan, Y. Labarga, L. Larizgoitia, L. Larumbe, A. Lebrun, P. Lopez, F. López-March, N. Madigan, R. Mano, R. D. P. Marques, A. P. Martín-Albo, J. Martínez-Lema, G. Martínez-Vara, M. Meziani, Z. E. Miller, R. L. Mistry, K. Molina-Canteras, J. Monrabal, F. Monteiro, C. M. B. Mora, F. J. Vidal, J. Muñoz Novella, P. Nuñez, A. Nygren, D. R. Oblak, E. Palacio, J. Palmeiro, B. Para, A. Parmaksiz, I. Pelegrin, J. Maneiro, M. Pérez Querol, M. Redwine, A. B. Renner, J. Rivilla, I. Rodríguez, J. Rogero, C. Rogers, L. Romeo, B. Romo-Luque, C. Santos, F. P. Santos, J. M. F. dos Shomroni, I. Simón, A. Soleti, S. R. Sorel, M. Soto-Oton, J. Teixeira, J. M. R. Toledo, J. F. Torrent, J. Trettin, A. Usón, A. Veloso, J. F. C. A. Waiton, J. White, J. T. High Energy Physics - Experiment Instrumentation and Detectors Noble element time projection chambers are a leading technology for rare event detection in physics, such as for dark matter and neutrinoless double beta decay searches. Time projection chambers typically assign event position in the drift direction using the relative timing of prompt scintillation and delayed charge collection signals, allowing for reconstruction of an absolute position in the drift direction. In this paper, alternate methods for assigning event drift distance via quantification of electron diffusion in a pure high pressure xenon gas time projection chamber are explored. Data from the NEXT-White detector demonstrate the ability to achieve good position assignment accuracy for both high- and low-energy events. Using point-like energy deposits from $^{83\mathrm{m}}$Kr calibration electron captures ($E\sim45$keV), the position of origin of low-energy events is determined to $2~$cm precision with bias $< 1$mm. A convolutional neural network approach is then used to quantify diffusion for longer tracks (E$\geq$1.5MeV), yielding a precision of 3cm on the event barycenter. The precision achieved with these methods indicates the feasibility energy calibrations of better than 1% FWHM at Q$_{ββ}$ in pure xenon, as well as the potential for event fiducialization in large future detectors using an alternate method that does not rely on primary scintillation.
title	Demonstration of Event Position Reconstruction based on Diffusion in the NEXT-White Detector
topic	High Energy Physics - Experiment Instrumentation and Detectors
url	https://arxiv.org/abs/2311.03441