Trends in Opioid Use Disorder in the Veterans Health Administration, 2005-2022
Gorfinkel, Lauren R; Malte, Carol A; Fink, David S; Mannes, Zachary L; Wall, Melanie M; Olfson, Mark; Livne, Ofir; Keyhani, Salomeh; Keyes, Katherine M; Martins, Silvia S; Cerdá, Magdalena; Gutkind, Sarah; Maynard, Charles C; Saxon, Andrew J; Simpson, Tracy; Gonsalves, Gregg; Lu, Haidong; McDowell, Yoanna; Hasin, Deborah S
IMPORTANCE/UNASSIGNED:Given the personal and social burdens of opioid use disorder (OUD), understanding time trends in OUD prevalence in large patient populations is key to planning prevention and treatment services. OBJECTIVE/UNASSIGNED:To examine trends in the prevalence of OUD from 2005 to 2022 overall and by age, sex, and race and ethnicity. DESIGN, SETTING, AND PARTICIPANTS/UNASSIGNED:This serial cross-sectional study included national Veterans Health Administration (VHA) electronic medical record data from the VHA Corporate Data Warehouse. Adult patients (age ≥18 years) with a current OUD diagnosis (using International Classification of Diseases, Ninth Revision, Clinical Modification [ICD-9-CM] and International Statistical Classification of Diseases, Tenth Revision, Clinical Modification [ICD-10-CM] codes) who received outpatient care at VHA facilities from January 1, 2005, to December 31, 2022, were eligible for inclusion in the analysis. MAIN OUTCOMES AND MEASURES/UNASSIGNED:The main outcome was OUD diagnoses. To test for changes in prevalence of OUD over time, multivariable logistic regression models were run that included categorical study year and were adjusted for sex, race and ethnicity, and categorical age. RESULTS/UNASSIGNED:The final sample size ranged from 4 332 165 to 5 962 564 per year; most were men (89.3%-95.0%). Overall, the annual percentage of VHA patients diagnosed with OUD almost doubled from 2005 to 2017 (0.60% [95% CI, 0.60%-0.61%] to 1.16% [95% CI, 1.15%-1.17%]; adjusted difference, 0.55 [95% CI, 0.54-0.57] percentage points) and declined thereafter (2022: 0.97% [95% CI, 0.97%-0.98%]; adjusted difference from 2017 to 2022, -0.18 [95% CI, -0.19 to -0.17] percentage points). This trend was similar among men (0.64% [95% CI, 0.63%-0.64%] in 2005 vs 1.22% [95% CI, 1.21%-1.23%] in 2017 vs 1.03% [95% CI, 1.02%-1.04%] in 2022), women (0.34% [95% CI, 0.32%-0.36%] in 2005 vs 0.68% [95% CI, 0.66%-0.69%] in 2017 vs 0.53% [95% CI, 0.52%-0.55%] in 2022), those younger than 35 years (0.62% [95% CI, 0.59%-0.66%] in 2005 vs 2.22% [95% CI, 2.18%-2.26%] in 2017 vs 1.00% [95% CI, 0.97%-1.03%] in 2022), those aged 35 to 64 years (1.21% [95% CI, 1.19%-1.22%] in 2005 vs 1.80% [95% CI, 1.78%-1.82%] in 2017 vs 1.41% [95% CI, 1.39%-1.42%] in 2022), and non-Hispanic White patients (0.44% [95% CI, 0.43%-0.45%] in 2005 vs 1.28% [95% CI, 1.27%-1.29%] in 2017 vs 1.13% [95% CI, 1.11%-1.14%] in 2022). Among VHA patients aged 65 years or older, OUD diagnoses increased from 2005 to 2022 (0.06% [95% CI, 0.06%-0.06%] to 0.61% [95% CI, 0.60%-0.62%]), whereas among Hispanic or Latino and non-Hispanic Black patients, OUD diagnoses decreased from 2005 (0.93% [95% CI, 0.88%-0.97%] and 1.26% [95% CI, 1.23%-1.28%], respectively) to 2022 (0.61% [95% CI, 0.59%-0.63%] and 0.82% [95% CI, 0.80%-0.83%], respectively). CONCLUSIONS AND RELEVANCE/UNASSIGNED:This serial cross-sectional study of national VHA electronic health record data found that the prevalence of OUD diagnoses increased from 2005 to 2017, peaked in 2017, and declined thereafter, a trend primarily attributable to changes among non-Hispanic White patients and those younger than 65 years. Continued public health efforts aimed at recognizing, treating, and preventing OUD are warranted.
PMCID:11662256
PMID: 39705031
ISSN: 2574-3805
CID: 5764912
Demonstrating Agreement between Radio and Fluorescence Measurements of the Depth of Maximum of Extensive Air Showers at the Pierre Auger Observatory
Abdul Halim, A; Abreu, P; Aglietta, M; Allekotte, I; Cheminant, K Almeida; Almela, A; Aloisio, R; Alvarez-Muñiz, J; Yebra, J Ammerman; Anastasi, G A; Anchordoqui, L; Andrada, B; Andringa, S; Anukriti,; Apollonio, L; Aramo, C; Ferreira, P R Araújo; Arnone, E; Velázquez, J C Arteaga; Assis, P; Avila, G; Avocone, E; Bakalova, A; Barbato, F; Mocellin, A Bartz; Bellido, J A; Berat, C; Bertaina, M E; Bhatta, G; Bianciotto, M; Biermann, P L; Binet, V; Bismark, K; Bister, T; Biteau, J; Blazek, J; Bleve, C; Blümer, J; Boháčová, M; Boncioli, D; Bonifazi, C; Arbeletche, L Bonneau; Borodai, N; Brack, J; Orchera, P G Brichetto; Briechle, F L; Bueno, A; Buitink, S; Buscemi, M; Büsken, M; Bwembya, A; Caballero-Mora, K S; Cabana-Freire, S; Caccianiga, L; Caruso, R; Castellina, A; Catalani, F; Cataldi, G; Cazon, L; Cerda, M; Cermenati, A; Chinellato, J A; Chudoba, J; Chytka, L; Clay, R W; Cerutti, A C Cobos; Colalillo, R; Coleman, A; Coluccia, M R; Conceição, R; Condorelli, A; Consolati, G; Conte, M; Convenga, F; Dos Santos, D Correia; Costa, P J; Covault, C E; Cristinziani, M; Sanchez, C S Cruz; Dasso, S; Daumiller, K; Dawson, B R; de Almeida, R M; de Jesús, J; de Jong, S J; Neto, J R T de Mello; De Mitri, I; de Oliveira, J; Franco, D de Oliveira; de Palma, F; de Souza, V; de Errico, B P de Souza; De Vito, E; Del Popolo, A; Deligny, O; Denner, N; Deval, L; di Matteo, A; Dobre, M; Dobrigkeit, C; D'Olivo, J C; Mendes, L M Domingues; Dorosti, Q; Dos Anjos, J C; Dos Anjos, R C; Ebr, J; Ellwanger, F; Emam, M; Engel, R; Epicoco, I; Erdmann, M; Etchegoyen, A; Evoli, C; Falcke, H; Farmer, J; Farrar, G; Fauth, A C; Fazzini, N; Feldbusch, F; Fenu, F; Fernandes, A; Fick, B; Figueira, J M; Filipčič, A; Fitoussi, T; Flaggs, B; Fodran, T; Fujii, T; Fuster, A; Galea, C; Galelli, C; García, B; Gaudu, C; Gemmeke, H; Gesualdi, F; Gherghel-Lascu, A; Ghia, P L; Giaccari, U; Glombitza, J; Gobbi, F; Gollan, F; Golup, G; Berisso, M Gómez; Vitale, P F Gómez; Gongora, J P; González, J M; González, N; Goos, I; Góra, D; Gorgi, A; Gottowik, M; Grubb, T D; Guarino, F; Guedes, G P; Guido, E; Gülzow, L; Hahn, S; Hamal, P; Hampel, M R; Hansen, P; Harari, D; Harvey, V M; Haungs, A; Hebbeker, T; Hojvat, C; Hörandel, J R; Horvath, P; Hrabovský, M; Huege, T; Insolia, A; Isar, P G; Janecek, P; Jilek, V; Johnsen, J A; Jurysek, J; Kampert, K-H; Keilhauer, B; Khakurdikar, A; Covilakam, V V Kizakke; Klages, H O; Kleifges, M; Knapp, F; Köhler, J; Kunka, N; Lago, B L; Langner, N; de Oliveira, M A Leigui; Lema-Capeans, Y; Letessier-Selvon, A; Lhenry-Yvon, I; Lopes, L; Lu, L; Luce, Q; Lundquist, J P; Payeras, A Machado; Majercakova, M; Mandat, D; Manning, B C; Mantsch, P; Marafico, S; Mariani, F M; Mariazzi, A G; Mariş, I C; Marsella, G; Martello, D; Martinelli, S; Bravo, O Martínez; Martins, M A; Mathes, H-J; Matthews, J; Matthiae, G; Mayotte, E; Mayotte, S; Mazur, P O; Medina-Tanco, G; Meinert, J; Melo, D; Menshikov, A; Merx, C; Michal, S; Micheletti, M I; Miramonti, L; Mollerach, S; Montanet, F; Morejon, L; Morello, C; Mulrey, K; Mussa, R; Namasaka, W M; Negi, S; Nellen, L; Nguyen, K; Nicora, G; Niechciol, M; Nitz, D; Nosek, D; Novotny, V; Nožka, L; Nucita, A; Núñez, L A; Oliveira, C; Palatka, M; Pallotta, J; Panja, S; Parente, G; Paulsen, T; Pawlowsky, J; Pech, M; Pękala, J; Pelayo, R; Pereira, L A S; Martins, E E Pereira; Armand, J Perez; Bertolli, C Pérez; Perrone, L; Petrera, S; Petrucci, C; Pierog, T; Pimenta, M; Platino, M; Pont, B; Pothast, M; Shahvar, M Pourmohammad; Privitera, P; Prouza, M; Puyleart, A; Querchfeld, S; Rautenberg, J; Ravignani, D; Akim, J V Reginatto; Reininghaus, M; Ridky, J; Riehn, F; Risse, M; Rizi, V; de Carvalho, W Rodrigues; Rodriguez, E; Rojo, J Rodriguez; Roncoroni, M J; Rossoni, S; Roth, M; Roulet, E; Rovero, A C; Ruehl, P; Saftoiu, A; Saharan, M; Salamida, F; Salazar, H; Salina, G; Gomez, J D Sanabria; Sánchez, F; Santos, E M; Santos, E; Sarazin, F; Sarmento, R; Sato, R; Savina, P; Schäfer, C M; Scherini, V; Schieler, H; Schimassek, M; Schimp, M; Schmidt, D; Scholten, O; Schoorlemmer, H; Schovánek, P; Schröder, F G; Schulte, J; Schulz, T; Sciutto, S J; Scornavacche, M; Segreto, A; Sehgal, S; Shivashankara, S U; Sigl, G; Silli, G; Sima, O; Simkova, K; Simon, F; Smau, R; Šmída, R; Sommers, P; Soriano, J F; Squartini, R; Stadelmaier, M; Stanič, S; Stasielak, J; Stassi, P; Strähnz, S; Straub, M; Suomijärvi, T; Supanitsky, A D; Svozilikova, Z; Szadkowski, Z; Tairli, F; Tapia, A; Taricco, C; Timmermans, C; Tkachenko, O; Tobiska, P; Peixoto, C J Todero; Tomé, B; Torrès, Z; Travaini, A; Travnicek, P; Trimarelli, C; Tueros, M; Unger, M; Vaclavek, L; Vacula, M; Galicia, J F Valdés; Valore, L; Varela, E; Vásquez-Ramírez, A; Veberič, D; Ventura, C; Quispe, I D Vergara; Verzi, V; Vicha, J; Vink, J; Vorobiov, S; Watanabe, C; Watson, A A; Weindl, A; Wiencke, L; Wilczyński, H; Wittkowski, D; Wundheiler, B; Yue, B; Yushkov, A; Zapparrata, O; Zas, E; Zavrtanik, D; Zavrtanik, M; ,
We show, for the first time, radio measurements of the depth of shower maximum (X_{max}) of air showers induced by cosmic rays that are compared to measurements of the established fluorescence method at the same location. Using measurements at the Pierre Auger Observatory we show full compatibility between our radio and the previously published fluorescence dataset, and between a subset of air showers observed simultaneously with both radio and fluorescence techniques, a measurement setup unique to the Pierre Auger Observatory. Furthermore, we show radio X_{max} resolution as a function of energy and demonstrate the ability to make competitive high-resolution X_{max} measurements with even a sparse radio array. With this, we show that the radio technique is capable of cosmic-ray mass composition studies, both at Auger and at other experiments.
PMID: 38277596
ISSN: 1079-7114
CID: 5911672