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Combined Annual Modulation Dark Matter Search with COSINE-100 and ANAIS-112

Fuente: arXiv

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Autores principales:	Carlin, N., Cho, J. Y., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Hong, S. B., Jeon, E. J., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Machado, V. H. A., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, H. K., Park, H. S., Park, J. C., Park, J. S., Park, K. S., Park, K., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Son, M. K., Spooner, N. J. C., Truc, L. T., Yang, L., Yu, G. H., Amaré, J., Apilluelo, J., Cebrián, S., Cintas, D., Coarasa, I., García, E., Martínez, M., Ortigoza, Y., de Solórzano, A. Ortiz, Pardo, T., Puimedón, J., Sarsa, M. L., Seoane, C.
Formato:	Preprint
Publicado:	2025
Materias:	Instrumentation and Methods for Astrophysics High Energy Physics - Experiment
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

_version_	1866911167174148096
author	Carlin, N. Cho, J. Y. Choi, J. J. Choi, S. Ezeribe, A. C. França, L. E. Ha, C. Hahn, I. S. Hollick, S. J. Hong, S. B. Jeon, E. J. Joo, H. W. Kang, W. G. Kauer, M. Kim, B. H. Kim, H. J. Kim, J. Kim, K. W. Kim, S. H. Kim, S. K. Kim, W. K. Kim, Y. D. Kim, Y. H. Ko, Y. J. Lee, D. H. Lee, E. K. Lee, H. Lee, H. S. Lee, H. Y. Lee, I. S. Lee, J. Lee, J. Y. Lee, M. H. Lee, S. H. Lee, S. M. Lee, Y. J. Leonard, D. S. Luan, N. T. Machado, V. H. A. Manzato, B. B. Maruyama, R. H. Neal, R. J. Olsen, S. L. Park, H. K. Park, H. S. Park, J. C. Park, J. S. Park, K. S. Park, K. Park, S. D. Pitta, R. L. C. Prihtiadi, H. Ra, S. J. Rott, C. Shin, K. A. Cavalcante, D. F. F. S. Son, M. K. Spooner, N. J. C. Truc, L. T. Yang, L. Yu, G. H. Amaré, J. Apilluelo, J. Cebrián, S. Cintas, D. Coarasa, I. García, E. Martínez, M. Ortigoza, Y. de Solórzano, A. Ortiz Pardo, T. Puimedón, J. Sarsa, M. L. Seoane, C.
author_facet	Carlin, N. Cho, J. Y. Choi, J. J. Choi, S. Ezeribe, A. C. França, L. E. Ha, C. Hahn, I. S. Hollick, S. J. Hong, S. B. Jeon, E. J. Joo, H. W. Kang, W. G. Kauer, M. Kim, B. H. Kim, H. J. Kim, J. Kim, K. W. Kim, S. H. Kim, S. K. Kim, W. K. Kim, Y. D. Kim, Y. H. Ko, Y. J. Lee, D. H. Lee, E. K. Lee, H. Lee, H. S. Lee, H. Y. Lee, I. S. Lee, J. Lee, J. Y. Lee, M. H. Lee, S. H. Lee, S. M. Lee, Y. J. Leonard, D. S. Luan, N. T. Machado, V. H. A. Manzato, B. B. Maruyama, R. H. Neal, R. J. Olsen, S. L. Park, H. K. Park, H. S. Park, J. C. Park, J. S. Park, K. S. Park, K. Park, S. D. Pitta, R. L. C. Prihtiadi, H. Ra, S. J. Rott, C. Shin, K. A. Cavalcante, D. F. F. S. Son, M. K. Spooner, N. J. C. Truc, L. T. Yang, L. Yu, G. H. Amaré, J. Apilluelo, J. Cebrián, S. Cintas, D. Coarasa, I. García, E. Martínez, M. Ortigoza, Y. de Solórzano, A. Ortiz Pardo, T. Puimedón, J. Sarsa, M. L. Seoane, C.
contents	The annual modulation signal, claimed to be consistent with dark matter as observed by DAMA/LIBRA in a sodium-iodide based detector, has persisted for over two decades. COSINE-100 and ANAIS-112 were designed to test the claim directly using the same target material. COSINE-100, located at Yangyang Underground Laboratory in South Korea, and ANAIS-112, located at Canfranc Underground Laboratory in Spain, have been taking data since 2016 and 2017, respectively. Each experiment published its respective results independently. In this paper, we present the results of an annual modulation search as a test of the signal observed by DAMA/LIBRA with the first three respective years of data from COSINE-100 and ANAIS-112. Using a Markov Chain Monte Carlo method, we find best fit values for modulation amplitude of $-0.0002 {\pm} 0.0026$ cpd/kg/keV in the 1-6 keV and $0.0021 {\pm} 0.0028$ cpd/kg/keV in the 2-6 keV energy regions. These results are not compatible with DAMA/LIBRA's assertion for their observation of annual modulation at $3.7σ$ and $2.6σ$, respectively. Performing a simple combination of the newly released 6-years datasets from both experiments find values consistent with no modulation at $0.0005 {\pm} 0.0019$ cpd/kg/keV in the 1-6 keV and $0.0027 {\pm} 0.0021$ cpd/kg/keV in the 2-6 keV energy regions with $4.68σ$ and $3.53σ$ respective exclusions of the DAMA/LIBRA signal.
format	Preprint
id	arxiv_https___arxiv_org_abs_2503_19559
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	Combined Annual Modulation Dark Matter Search with COSINE-100 and ANAIS-112 Carlin, N. Cho, J. Y. Choi, J. J. Choi, S. Ezeribe, A. C. França, L. E. Ha, C. Hahn, I. S. Hollick, S. J. Hong, S. B. Jeon, E. J. Joo, H. W. Kang, W. G. Kauer, M. Kim, B. H. Kim, H. J. Kim, J. Kim, K. W. Kim, S. H. Kim, S. K. Kim, W. K. Kim, Y. D. Kim, Y. H. Ko, Y. J. Lee, D. H. Lee, E. K. Lee, H. Lee, H. S. Lee, H. Y. Lee, I. S. Lee, J. Lee, J. Y. Lee, M. H. Lee, S. H. Lee, S. M. Lee, Y. J. Leonard, D. S. Luan, N. T. Machado, V. H. A. Manzato, B. B. Maruyama, R. H. Neal, R. J. Olsen, S. L. Park, H. K. Park, H. S. Park, J. C. Park, J. S. Park, K. S. Park, K. Park, S. D. Pitta, R. L. C. Prihtiadi, H. Ra, S. J. Rott, C. Shin, K. A. Cavalcante, D. F. F. S. Son, M. K. Spooner, N. J. C. Truc, L. T. Yang, L. Yu, G. H. Amaré, J. Apilluelo, J. Cebrián, S. Cintas, D. Coarasa, I. García, E. Martínez, M. Ortigoza, Y. de Solórzano, A. Ortiz Pardo, T. Puimedón, J. Sarsa, M. L. Seoane, C. Instrumentation and Methods for Astrophysics High Energy Physics - Experiment The annual modulation signal, claimed to be consistent with dark matter as observed by DAMA/LIBRA in a sodium-iodide based detector, has persisted for over two decades. COSINE-100 and ANAIS-112 were designed to test the claim directly using the same target material. COSINE-100, located at Yangyang Underground Laboratory in South Korea, and ANAIS-112, located at Canfranc Underground Laboratory in Spain, have been taking data since 2016 and 2017, respectively. Each experiment published its respective results independently. In this paper, we present the results of an annual modulation search as a test of the signal observed by DAMA/LIBRA with the first three respective years of data from COSINE-100 and ANAIS-112. Using a Markov Chain Monte Carlo method, we find best fit values for modulation amplitude of $-0.0002 {\pm} 0.0026$ cpd/kg/keV in the 1-6 keV and $0.0021 {\pm} 0.0028$ cpd/kg/keV in the 2-6 keV energy regions. These results are not compatible with DAMA/LIBRA's assertion for their observation of annual modulation at $3.7σ$ and $2.6σ$, respectively. Performing a simple combination of the newly released 6-years datasets from both experiments find values consistent with no modulation at $0.0005 {\pm} 0.0019$ cpd/kg/keV in the 1-6 keV and $0.0027 {\pm} 0.0021$ cpd/kg/keV in the 2-6 keV energy regions with $4.68σ$ and $3.53σ$ respective exclusions of the DAMA/LIBRA signal.
title	Combined Annual Modulation Dark Matter Search with COSINE-100 and ANAIS-112
topic	Instrumentation and Methods for Astrophysics High Energy Physics - Experiment
url	https://arxiv.org/abs/2503.19559