1,667 results on '"Bustamante, M"'
Search Results
2. Effect of impeller type on cellular morphology and production of clavulanic acid by Streptomyces clavuligerus
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Bustamante, M. C. C., Costa, C. L. L., Esperança, M. N., Mazziero, V. T., Cerri, M. O., and Badino, Alberto C.
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- 2024
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3. Evaluation of aldosterone to direct renin ratio, low renin and related Phenotypes in Afro-Colombian patients with apparent treatment resistant hypertension
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Durán, C. E., Bustamante, M., Barbosa, M., Useche, E. M., Triviño, J., Sandoval, L., Moncayo, P. A., Rivas, A. M., Zapata, J. S., Hernández Quintero, J. D., Meza, S., Bolaños, J. S., Schweineberg, J., Mesa, L., and Posada, J. G.
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- 2024
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4. The Milky Way shines in high-energy neutrinos
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Bustamante, M.
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- 2024
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5. Amphibia, Centrolenidae, Cochranella pulverata, Hyalinobatrachium aureoguttatum: Distribution extension, Ecuador.
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Bustamante, M. R., Cisneros-Heredia, D. F., Yánez-Muñoz, M. H., Ortega-Andrade, H. M., and Guayasamin, J. M.
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Biology (General) ,QH301-705.5 - Published
- 2007
6. Snowmass White Paper: Beyond the Standard Model effects on Neutrino Flavor
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Argüelles, C. A., Barenboim, G., Bustamante, M., Coloma, P., Denton, P. B., Esteban, I., Farzan, Y., Martínez, E. Fernández, Forero, D. V., Gago, A. M., Katori, T., Lehnert, R., Ross-Lonergan, M., Suliga, A. M., Tabrizi, Z., Anchordoqui, L., Chakraborty, K., Conrad, J., Das, A., Fong, C. S., Littlejohn, B. R., Maltoni, M., Parno, D., Spitz, J., Tang, J., and Wissel, S.
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High Energy Physics - Phenomenology ,High Energy Physics - Experiment - Abstract
Neutrinos are one of the most promising messengers for signals of new physics Beyond the Standard Model (BSM). On the theoretical side, their elusive nature, combined with their unknown mass mechanism, seems to indicate that the neutrino sector is indeed opening a window to new physics. On the experimental side, several long-standing anomalies have been reported in the past decades, providing a strong motivation to thoroughly test the standard three-neutrino oscillation paradigm. In this Snowmass21 white paper, we explore the potential of current and future neutrino experiments to explore BSM effects on neutrino flavor during the next decade., Comment: 54 pages plus references. Contact authors: P. Coloma, D. V. Forero and T. Katori. Comments welcome. Contribution to Snowmass 2021. v2 incorporates community feedback
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- 2022
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7. Identifying the circularization opportunities for organic wastes generated in a Mediterranean region
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García-Rández, A., Marks, E. A. N., Martínez-Sabater, E., Sáez-Tovar, J. A., Andreu-Rodríguez, J., Orden, L., Bustamante, M. A., Pérez-Murcia, M. D., and Moral, R.
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- 2023
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8. EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade
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Batista, R. Alves, Amin, M. A., Barenboim, G., Bartolo, N., Baumann, D., Bauswein, A., Bellini, E., Benisty, D., Bertone, G., Blasi, P., Böhmer, C. G., Bošnjak, Ž., Bringmann, T., Burrage, C., Bustamante, M., Bustillo, J. Calderón, Byrnes, C. T., Calore, F., Catena, R., Cerdeño, D. G., Cerri, S. S., Chianese, M., Clough, K., Cole, A., Coloma, P., Coogan, A., Covi, L., Cutting, D., Davis, A. C., de Rham, C., di Matteo, A., Domènech, G., Drewes, M., Dietrich, T., Edwards, T. D. P., Esteban, I., Erdem, R., Evoli, C., Fasiello, M., Feeney, S. M., Ferreira, R. Z., Fialkov, A., Fornengo, N., Gabici, S., Galatyuk, T., Gaggero, D., Grasso, D., Guépin, C., Harz, J., Herrero-Valea, M., Hinderer, T., Hogg, N. B., Hooper, D. C., Iocco, F., Isern, J., Karchev, K., Kavanagh, B. J., Korsmeier, M., Kotera, K., Koyama, K., Krishnan, B., Lesgourgues, J., Said, J. Levi, Lombriser, L., Lorenz, C. S., Manconi, S., Mapelli, M., Marcowith, A., Markoff, S. B., Marsh, D. J. E., Martinelli, M., Martins, C. J. A. P., Matthews, J. H., Meli, A., Mena, O., Mifsud, J., Bertolami, M. M. Miller, Millington, P., Moesta, P., Nippel, K., Niro, V., O'Connor, E., Oikonomou, F., Paganini, C. F., Pagliaroli, G., Pani, P., Pfrommer, C., Pascoli, S., Pinol, L., Pizzuti, L., Porto, R. A., Pound, A., Quevedo, F., Raffelt, G. G., Raccanelli, A., Ramirez-Ruiz, E., Raveri, M., Renaux-Petel, S., Ricciardone, A., Khalifeh, A. Rida, Riotto, A., Roiban, R., Rubio, J., Sahlén, M., Sabti, N., Sagunski, L., Šarčević, N., Schmitz, K., Schwaller, P., Schwetz, T., Sedrakian, A., Sellentin, E., Serenelli, A., Serpico, P. D., Sfakianakis, E. I., Shalgar, S., Silvestri, A., Tamborra, I., Tanidis, K., Teresi, D., Tokareva, A. A., Tolos, L., Trojanowski, S., Trotta, R., Uhlemann, C., Urban, F. R., Vernizzi, F., van Vliet, A., Villante, F. L., Vincent, A., Vink, J., Vitagliano, E., Weniger, C., Wickenbrock, A., Winter, W., Zell, S., and Zeng, M.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Astroparticle physics is undergoing a profound transformation, due to a series of extraordinary new results, such as the discovery of high-energy cosmic neutrinos with IceCube, the direct detection of gravitational waves with LIGO and Virgo, and many others. This white paper is the result of a collaborative effort that involved hundreds of theoretical astroparticle physicists and cosmologists, under the coordination of the European Consortium for Astroparticle Theory (EuCAPT). Addressed to the whole astroparticle physics community, it explores upcoming theoretical opportunities and challenges for our field of research, with particular emphasis on the possible synergies among different subfields, and the prospects for solving the most fundamental open questions with multi-messenger observations., Comment: White paper of the European Consortium for Astroparticle Theory (EuCAPT). 135 authors, 400 endorsers, 133 pages, 1382 references
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- 2021
9. The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory
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Olinto, A. V., Krizmanic, J., Adams, J. H., Aloisio, R., Anchordoqui, L. A., Anzalone, A., Bagheri, M., Barghini, D., Battisti, M., Bergman, D. R., Bertaina, M. E., Bertone, P. F., Bisconti, F., Bustamante, M., Cafagna, F., Caruso, R., Casolino, M., Černý, K., Christl, M. J., Cummings, A. L., De Mitri, I., Diesing, R., Engel, R., Eser, J., Fang, K., Fenu, F., Filippatos, G., Gazda, E., Guepin, C., Haungs, A., Hays, E. A., Judd, E. G., Klimov, P., Kungel, V., Kuznetsov, E., Mackovjak, Š., Mandát, D., Marcelli, L., McEnery, J., Medina-Tanco, G., Merenda, K. -D., Meyer, S. S., Mitchell, J. W., Miyamoto, H., Nachtman, J. M., Neronov, A., Oikonomou, F., Onel, Y., Osteria, G., Otte, A. N., Parizot, E., Paul, T., Pech, M., Perkins, J. S., Picozza, P., Piotrowski, L. W., Plebaniak, Z., Prévôt, G., Reardon, P., Reno, M. H., Ricci, M., Matamala, O. Romero, Sarazin, F., Schovánek, P., Scotti, V., Shinozaki, K., Soriano, J. F., Stecker, F., Takizawa, Y., Ulrich, R., Unger, M., Venters, T. M., Wiencke, L., Winn, D., Young, R. M., and Zotov, M.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,High Energy Physics - Experiment - Abstract
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to accurately observe ultra-high-energy cosmic rays (UHECRs) and cosmic neutrinos from space with sensitivity over the full celestial sky. POEMMA will observe the extensive air showers (EASs) from UHECRs and UHE neutrinos above 20 EeV via air fluorescence. Additionally, POEMMA will observe the Cherenkov signal from upward-moving EASs induced by Earth-interacting tau neutrinos above 20 PeV. The POEMMA spacecraft are designed to quickly re-orientate to follow up transient neutrino sources and obtain unparalleled neutrino flux sensitivity. Developed as a NASA Astrophysics Probe-class mission, POEMMA consists of two identical satellites flying in loose formation in 525 km altitude orbits. Each POEMMA instrument incorporates a wide field-of-view (45$^\circ$) Schmidt telescope with over 6 m$^2$ of collecting area. The hybrid focal surface of each telescope includes a fast (1~$\mu$s) near-ultraviolet camera for EAS fluorescence observations and an ultrafast (10~ns) optical camera for Cherenkov EAS observations. In a 5-year mission, POEMMA will provide measurements that open new multi-messenger windows onto the most energetic events in the universe, enabling the study of new astrophysics and particle physics at these otherwise inaccessible energies., Comment: 66 pages, 53 figures; JCAP accepted version
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- 2020
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10. Snowmass 2021 Letter of Interest: The Probe Of Multi-Messenger Astrophysics (POEMMA)
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Olinto, A. V., Sarazin, F., Adams, J. H., Aloisio, R., Anchordoqui, L. A., Bagheri, M., Barghini, D., Battisti, M., Bergman, D. R., Bertaina, M. E., Bertone, P. F., Bisconti, F., Bustamante, M., Casolino, M., Christl, M. J., Cummings, A. L., De Mitri, I., Diesing, R., Engel, R., Eser, J., Fang, K., Fillipatos, G., Fenu, F., Gazda, E., Guepin, C., Hays, E. A., Judd, E. G., Klimov, P., Krizmanic, J., Kungel, V., Kuznetsov, E., Mackovjak, S., Marcelli, L., McEnery, J., Merenda, K. -D., Meyer, S. S., Mitchell, J. W., Miyamoto, H., Nachtman, J. M., Neronov, A., Oikonomou, F., Onel, Y., Otte, A. N., Parizot, E., Paul, T., Perkins, J. S., Picozza, P., Piotrowski, L. W., Prevot, G., Reardon, P., Reno, M. H., Ricci, M., Matamala, O. Romero, Shinozaki, K., Soriano, J. F., Stecker, F., Takizawa, Y., Ulrich, R., Unger, M., Venters, T. M., Wiencke, L., Winn, D., Young, R. M., and Zotov, M.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to identify the sources of Ultra-High-Energy Cosmic Rays (UHECRs) and to observe cosmic neutrinos, both with full-sky coverage. Developed as a NASA Astrophysics Probe-class mission, POEMMA consists of two spacecraft flying in a loose formation at 525 km altitude, 28.5 deg inclination orbits. Each spacecraft hosts a Schmidt telescope with a large collecting area and wide field of view. A novel focal plane is optimized to observe both the UV fluorescence signal from extensive air showers (EASs) and the beamed optical Cherenkov signals from EASs. In POEMMA-stereo fluorescence mode, POEMMA will measure the spectrum, composition, and full-sky distribution of the UHECRs above 20 EeV with high statistics along with remarkable sensitivity to UHE neutrinos. The spacecraft are designed to quickly re-orient to a POEMMA-limb mode to observe neutrino emission from Target-of-Opportunity (ToO) transient astrophysical sources viewed just below the Earth's limb. In this mode, POEMMA will have unique sensitivity to cosmic neutrino tau events above 20 PeV by measuring the upward-moving EASs induced by the decay of the emerging tau leptons following the interactions of neutrino tau inside the Earth., Comment: 3 pages, no figures, LoI for Snowmass 2021
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- 2020
11. IceCube-Gen2: The Window to the Extreme Universe
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Collaboration, The IceCube-Gen2, Aartsen, M. G., Abbasi, R., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Alispach, C., Allison, P., Amin, N. M., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Arlen, T. C., Auffenberg, J., Axani, S., Bagherpour, H., Bai, X., V., A. Balagopal, Barbano, A., Bartos, I., Bastian, B., Basu, V., Baum, V., Baur, S., Bay, R., Beatty, J. J., Becker, K. -H., Tjus, J. Becker, BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Bohmer, M., Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bron, S., Brostean-Kaiser, J., Burgman, A., Burley, R. T., Buscher, J., Busse, R. S., Bustamante, M., Campana, M. A., Carnie-Bronca, E. G., Carver, T., Chen, C., Chen, P., Cheung, E., Chirkin, D., Choi, S., Clark, B. A., Clark, K., Classen, L., Coleman, A., Collin, G. H., Connolly, A., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., Deaconu, C., De Clercq, C., DeLaunay, J. J., De Kockere, S., Dembinski, H., Deoskar, K., De Ridder, S., Desai, A., Desiati, P., de Vries, K. D., de Wasseige, G., de With, M., DeYoung, T., Dharani, S., Diaz, A., Díaz-Vélez, J. C., Dujmovic, H., Dunkman, M., DuVernois, M. A., Dvorak, E., Ehrhardt, T., Eller, P., Engel, R., Evans, J. J., Evenson, P. A., Fahey, S., Farrag, K., Fazely, A. R., Felde, J., Fienberg, A. T., Filimonov, K., Finley, C., Fischer, L., Fox, D., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K., Gallagher, J., Ganster, E., Garcia-Fernandez, D., Garrappa, S., Gartner, A., Gerhardt, L., Gernhaeuser, R., Ghadimi, A., Glaser, C., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Goswami, S., Grant, D., Grégoire, T., Griffith, Z., Griswold, S., Gündüz, M., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Hanson, J. C., Hanson, K., Hardin, J., Haugen, J., Haungs, A., Hauser, S., Hebecker, D., Heinen, D., Heix, P., Helbing, K., Hellauer, R., Henningsen, F., Hickford, S., Hignight, J., Hill, C., Hill, G. C., Hoffman, K. D., Hoffmann, B., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Holzapfel, K., Hoshina, K., Huang, F., Huber, M., Huber, T., Huege, T., Hughes, K., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jansson, M., Japaridze, G. S., Jeong, M., Jones, B. J. P., Jonske, F., Joppe, R., Kalekin, O., Kang, D., Kang, W., Kang, X., Kappes, A., Kappesser, D., Karg, T., Karl, M., Karle, A., Katori, T., Katz, U., Kauer, M., Keivani, A., Kellermann, M., Kelley, J. L., Kheirandish, A., Kim, J., Kin, K., Kintscher, T., Kiryluk, J., Kittler, T., Kleifges, M., Klein, S. R., Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Koundal, P., Kovacevich, M., Kowalski, M., Krauss, C. B., Krings, K., Krückl, G., Kulacz, N., Kurahashi, N., Gualda, C. Lagunas, Lahmann, R., Lanfranchi, J. L., Larson, M. J., Latif, U., Lauber, F., Lazar, J. P., Leonard, K., Leszczyńska, A., Li, Y., Liu, Q. R., Lohfink, E., LoSecco, J., Mariscal, C. J. Lozano, Lu, L., Lucarelli, F., Ludwig, A., Lünemann, J., Luszczak, W., Lyu, Y., Ma, W. Y., Madsen, J., Maggi, G., Mahn, K. B. M., Makino, Y., Mallik, P., Mancina, S., Mandalia, S., Mariş, I. C., Marka, S., Marka, Z., Maruyama, R., Mase, K., Maunu, R., McNally, F., Meagher, K., Medina, A., Meier, M., Meighen-Berger, S., Merz, J., Meyers, Z. S., Micallef, J., Mockler, D., Momenté, G., Montaruli, T., Moore, R. W., Morse, R., Moulai, M., Muth, P., Naab, R., Nagai, R., Nam, J., Naumann, U., Necker, J., Neer, G., Nelles, A., Nguyên, L. V., Niederhausen, H., Nisa, M. U., Nowicki, S. C., Nygren, D. R., Oberla, E., Pollmann, A. Obertacke, Oehler, M., Olivas, A., O'Sullivan, E., Pan, Y., Pandya, H., Pankova, D. V., Papp, L., Park, N., Parker, G. K., Paudel, E. N., Peiffer, P., Heros, C. Pérez de los, Petersen, T. C., Philippen, S., Pieloth, D., Pieper, S., Pinfold, J. L., Pizzuto, A., Plaisier, I., Plum, M., Popovych, Y., Porcelli, A., Rodriguez, M. Prado, Price, P. B., Przybylski, G. T., Raab, C., Raissi, A., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C., Rehman, A., Reimann, R., Renschler, M., Renzi, G., Resconi, E., Reusch, S., Rhode, W., Richman, M., Riedel, B., Riegel, M., Roberts, E. J., Robertson, S., Roellinghoff, G., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Cantu, D. Rysewyk, Safa, I., Herrera, S. E. Sanchez, Sandrock, A., Sandroos, J., Sandstrom, P., Santander, M., Sarkar, S., Satalecka, K., Scharf, M., Schaufel, M., Schieler, H., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Shaevitz, M. H., Sharma, A., Shefali, S., Silva, M., Smith, D., Smithers, B., Snihur, R., Soedingrekso, J., Soldin, D., Söldner-Rembold, S., Song, M., Southall, D., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stein, R., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Strotjohann, N. L., Stürwald, T., Stuttard, T., Sullivan, G. W., Taboada, I., Taketa, A., Tanaka, H. K. M., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Tollefson, K., Tomankova, L., Tönnis, C., Torres, J., Toscano, S., Tosi, D., Trettin, A., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Twagirayezu, J. P., Ty, B., Unger, E., Elorrieta, M. A. Unland, Vandenbroucke, J., van Eijk, D., van Eijndhoven, N., Vannerom, D., van Santen, J., Veberic, D., Verpoest, S., Vieregg, A., Vraeghe, M., Walck, C., Watson, T. B., Weaver, C., Weindl, A., Weinstock, L., Weiss, M. J., Weldert, J., Welling, C., Wendt, C., Werthebach, J., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissel, S. A., Wolf, M., Wood, T. R., Woschnagg, K., Wrede, G., Wren, S., Wulff, J., Xu, X. W., Xu, Y., Yanez, J. P., Yoshida, S., Yuan, T., Zhang, Z., Zierke, S., and Zöcklein, M.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. The discovery of cosmic neutrinos with IceCube has opened this new window on the universe. In this white paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the processes and environments that govern the universe at the highest energies. IceCube-Gen2 is designed to: 1) Resolve the high-energy neutrino sky from TeV to EeV energies; 2) Investigate cosmic particle acceleration through multi-messenger observations; 3) Reveal the sources and propagation of the highest energy particles in the universe; 4) Probe fundamental physics with high-energy neutrinos. IceCube-Gen2 will increase the annual rate of observed cosmic neutrinos by a factor of ten compared to IceCube, and will be able to detect sources five times fainter than its predecessor. Furthermore, through the addition of a radio array, IceCube-Gen2 will extend the energy range by several orders of magnitude compared to IceCube. Construction will take 8 years and cost about \$350M. The goal is to have IceCube-Gen2 fully operational by 2033. IceCube-Gen2 will play an essential role in shaping the new era of multi-messenger astronomy, fundamentally advancing our knowledge of the high-energy universe. This challenging mission can be fully addressed only in concert with the new survey instruments across the electromagnetic spectrum and gravitational wave detectors which will be available in the coming years., Comment: 56 pages, 29 figures
- Published
- 2020
- Full Text
- View/download PDF
12. IceCube-Gen2: the window to the extreme Universe
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Aartsen, MG, Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alispach, C, Allison, P, Amin, NM, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Arlen, TC, Auffenberg, J, Axani, S, Bagherpour, H, Bai, X, Balagopal, A, Barbano, A, Bartos, I, Bastian, B, Basu, V, Baum, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Bohmer, M, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Burgman, A, Burley, RT, Buscher, J, Busse, RS, Bustamante, M, Campana, MA, Carnie-Bronca, EG, Carver, T, Chen, C, Chen, P, Cheung, E, Chirkin, D, Choi, S, Clark, BA, Clark, K, Classen, L, Coleman, A, Collin, GH, Connolly, A, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, Deaconu, C, De Clercq, C, DeLaunay, JJ, De Kockere, S, Dembinski, H, Deoskar, K, De Ridder, S, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Dharani, S, Diaz, A, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, DuVernois, MA, Dvorak, E, Ehrhardt, T, Eller, P, Engel, R, Evans, JJ, and Evenson, PA
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neutrino astronomy ,high-energy astrophysics ,neutrino telescopes ,astro-ph.HE ,Atomic ,Molecular ,Nuclear ,Particle and Plasma Physics ,Nuclear & Particles Physics - Abstract
The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a wealth of information about the Universe. However, at PeV (1015 eV) energies and above, most of the Universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the Universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. These energetic particles havemillions of times higher energies than those produced in the most powerful particle accelerators on Earth. As neutrinos can escape from regions otherwise opaque to radiation, they allow an unique view deep into exploding stars and the vicinity of the event horizons of black holes. The discovery of cosmic neutrinos with IceCube has opened this new window on the Universe. IceCube has been successful in finding first evidence for cosmic particle acceleration in the jet of an active galactic nucleus. Yet, ultimately, its sensitivity is too limited to detect even the brightest neutrino sources with high significance, or to detect populations of less luminous sources. In thiswhite paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the processes and environments that govern the Universe at the highest energies. IceCube-Gen2 is designed to: (a) Resolve the high-energy neutrino sky from TeV to EeV energies (b) Investigate cosmic particle acceleration through multi-messenger observations (c) Reveal the sources and propagation of the highest energy particles in the Universe (d) Probe fundamental physics with high-energy neutrinos IceCube-Gen2 will enhance the existing IceCube detector at the South Pole. It will increase the annual rate of observed cosmic neutrinos by a factor of ten compared to IceCube, and will be able to detect sources five times fainter than its predecessor. Furthermore, through the addition of a radio array, IceCube- Gen2 will extend the energy range by several orders of magnitude compared to IceCube. Construction will take 8 years and cost about $350M. The goal is to have IceCube-Gen2 fully operational by 2033. IceCube-Gen2 will play an essential role in shaping the new era of multimessenger astronomy, fundamentally advancing our knowledge of the highenergy Universe. This challenging mission can be fully addressed only through the combination of the information from the neutrino, electromagnetic, and gravitational wave emission of high-energy sources, in concert with the new survey instruments across the electromagnetic spectrum and gravitational wave detectors which will be available in the coming years.
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- 2021
13. Neutrino astronomy with the next generation IceCube Neutrino Observatory
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Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Alispach, C., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Arlen, T. C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., V., A. Balagopal, Barbano, A., Bartos, I., Bastian, B., Baum, V., Baur, S., Bay, R., Beatty, J. J., Becker, K. -H., Tjus, J. Becker, BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Bohmer, M., Börner, M., Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bron, S., Brostean-Kaiser, J., Burgman, A., Buscher, J., Busse, R. S., Bustamante, M., Carver, T., Chen, C., Chen, P., Cheung, E., Chirkin, D., Clark, B., Clark, K., Classen, L., Coleman, A., Collin, G. H., Connolly, A., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., Deaconu, C., de André, J. P. A. M., De Clercq, C., DeKockere, S., DeLaunay, J. J., Dembinski, H., Deoskar, K., De Ridder, S., Desiati, P., de Vries, K. D., de Wasseige, G., de With, M., DeYoung, T., Diaz, A., Díaz-Vélez, J. C., Dujmovic, H., Dunkman, M., DuVernois, M. A., Dvorak, E., Eberhardt, B., Ehrhardt, T., Eller, P., Engel, R., Evans, J. J., Evenson, P. A., Fahey, S., Farrag, K., Fazely, A. R., Felde, J., Filimonov, K., Finley, C., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K., Gallagher, J., Ganster, E., Garcia-Fernandez, D., Garrappa, S., Gartner, A., Gerhardt, L., Gernhaeuser, R., Ghorbani, K., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Griffith, Z., Günder, M., Gündüz, M., Haack, C., Hallgren, A., Halve, L., Halzen, F., Hanson, K., Haugen, J., Haungs, A., Hebecker, D., Heereman, D., Heix, P., Helbing, K., Hellauer, R., Henningsen, F., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, B., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Holzapfel, K., Hoshina, K., Huang, F., Huber, M., Huber, T., Huege, T., Hughes, K., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Jonske, F., Joppe, R., Kalekin, O., Kang, D., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karl, M., Karle, A., Katori, T., Katz, U., Kauer, M., Keivani, A., Kelley, J. L., Kheirandish, A., Kim, J., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krauss, C. B., Krings, K., Krückl, G., Kulacz, N., Kurahashi, N., Kyriacou, A., Labare, M., Lanfranchi, J. L., Larson, M. J., Latif, U., Lauber, F., Lazar, J. P., Leonard, K., Leszczynska, A., Leuermann, M., Liu, Q. R., Lohfink, E., LoSecco, J., Mariscal, C. J. Lozano, Lu, L., Lucarelli, F., Lünemann, J., Luszczak, W., Lyu, Y., Ma, W. Y., Madsen, J., Maggi, G., Mahn, K. B. M., Makino, Y., Mallik, P., Mallot, K., Mancina, S., Mandalia, S., Maris, I. C., Marka, S., Marka, Z., Maruyama, R., Mase, K., Maunu, R., McNally, F., Meagher, K., Medici, M., Medina, A., Meier, M., Meighen-Berger, S., Menne, T., Merino, G., Meures, T., Micallef, J., Momenté, G., Montaruli, T., Moore, R. W., Morse, R., Moulai, M., Muth, P., Nagai, R., Nam, J., Naumann, U., Neer, G., Nelles, A., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Pollmann, A. Obertacke, Oehler, M., Olivas, A., O'Murchadha, A., O'Sullivan, E., Palczewski, T., Pandya, H., Pankova, D. V., Papp, L., Park, N., Peiffer, P., Heros, C. Pérez de los, Petersen, T. C., Philippen, S., Pieloth, D., Pinat, E., Pinfold, J. L., Pizzuto, A., Plaisier, I., Plum, M., Porcelli, A., Price, P. B., Przybylski, G. T., Raab, C., Raissi, A., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C., Reimann, R., Relethford, B., Renschler, M., Renzi, G., Resconi, E., Rhode, W., Richman, M., Riegel, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Safa, I., Herrera, S. E. Sanchez, Sandrock, A., Sandroos, J., Sandstrom, P., Santander, M., Sarkar, S., Satalecka, K., Schaufel, M., Schieler, H., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Shaevitz, M. H., Shefali, S., Silva, M., Smith, D., Snihur, R., Soedingrekso, J., Soldin, D., Söldner-Rembold, S., Song, M., Southall, D., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stein, R., Steinmüller, P., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strotjohann, N. L., Stürwald, T., Stuttard, T., Sullivan, G. W., Taboada, I., Taketa, A., Tanaka, H. K. M., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Tomankova, L., Tönnis, C., Torres, J., Toscano, S., Tosi, D., Trettin, A., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Ty, B., Unger, E., Elorrieta, M. A. Unland, Usner, M., Vandenbroucke, J., Van Driessche, W., van Eijk, D., van Eijndhoven, N., Vanheule, S., Vieregg, A., van Santen, J., Veberic, D., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandkowsky, N., Watson, T. B., Weaver, C., Weindl, A., Weiss, M. J., Weldert, J., Welling, C., Wendt, C., Werthebach, J., Whelan, B. J., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wissel, S., Wolf, M., Wood, J., Wood, T. R., Woschnagg, K., Wrede, G., Wren, S., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Yuan, T., and Zöcklein, M.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The past decade has welcomed the emergence of cosmic neutrinos as a new messenger to explore the most extreme environments of the universe. The discovery measurement of cosmic neutrinos, announced by IceCube in 2013, has opened a new window of observation that has already resulted in new fundamental information that holds the potential to answer key questions associated with the high-energy universe, including: what are the sources in the PeV sky and how do they drive particle acceleration; where are cosmic rays of extreme energies produced, and on which paths do they propagate through the universe; and are there signatures of new physics at TeV-PeV energies and above? The planned advancements in neutrino telescope arrays in the next decade, in conjunction with continued progress in broad multimessenger astrophysics, promise to elevate the cosmic neutrino field from the discovery to the precision era and to a survey of the sources in the neutrino sky. The planned detector upgrades to the IceCube Neutrino Observatory, culminating in IceCube-Gen2 (an envisaged $400M facility with anticipated operation in the next decade, described in this white paper) are the cornerstone that will drive the evolution of neutrino astrophysics measurements., Comment: related submission to Astro2020 decadal survey
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- 2019
14. Development of a small panel of SNPs to infer ancestry in Chileans that distinguishes Aymara and Mapuche components
- Author
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Verdugo, Ricardo A, Di Genova, Alex, Herrera, Luisa, Moraga, Mauricio, Acuña, Mónica, Berríos, Soledad, Llop, Elena, Valenzuela, Carlos Y, Bustamante, M Leonor, Digman, Dayhana, Symon, Adriana, Asenjo, Soledad, López, Pamela, Blanco, Alejandro, Suazo, José, Barozet, Emmanuelle, Caba, Fresia, Villalón, Marcelo, Alvarado, Sergio, Cáceres, Dante, Salgado, Katherine, Portales, Pilar, Moreno-Estrada, Andrés, Gignoux, Christopher R, Sandoval, Karla, Bustamante, Carlos D, Eng, Celeste, Huntsman, Scott, Burchard, Esteban G, Loira, Nicolás, Maass, Alejandro, and Cifuentes, Lucía
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Chile ,Ethnicity ,Female ,Gene Frequency ,Genetic Markers ,Genetics ,Population ,Genotype ,Genotyping Techniques ,Humans ,Indians ,South American ,Male ,Phylogeography ,Polymorphism ,Single Nucleotide ,Population Groups ,Saliva ,Admixture ,Ancestry ,Aymara ,Mapuche ,SNPs panel ,Biological Sciences ,Biochemistry & Molecular Biology - Abstract
BackgroundCurrent South American populations trace their origins mainly to three continental ancestries, i.e. European, Amerindian and African. Individual variation in relative proportions of each of these ancestries may be confounded with socio-economic factors due to population stratification. Therefore, ancestry is a potential confounder variable that should be considered in epidemiologic studies and in public health plans. However, there are few studies that have assessed the ancestry of the current admixed Chilean population. This is partly due to the high cost of genome-scale technologies commonly used to estimate ancestry. In this study we have designed a small panel of SNPs to accurately assess ancestry in the largest sampling to date of the Chilean mestizo population (n = 3349) from eight cities. Our panel is also able to distinguish between the two main Amerindian components of Chileans: Aymara from the north and Mapuche from the south.ResultsA panel of 150 ancestry-informative markers (AIMs) of SNP type was selected to maximize ancestry informativeness and genome coverage. Of these, 147 were successfully genotyped by KASPar assays in 2843 samples, with an average missing rate of 0.012, and a 0.95 concordance with microarray data. The ancestries estimated with the panel of AIMs had relative high correlations (0.88 for European, 0.91 for Amerindian, 0.70 for Aymara, and 0.68 for Mapuche components) with those obtained with AXIOM LAT1 array. The country's average ancestry was 0.53 ± 0.14 European, 0.04 ± 0.04 African, and 0.42 ± 0.14 Amerindian, disaggregated into 0.18 ± 0.15 Aymara and 0.25 ± 0.13 Mapuche. However, Mapuche ancestry was highest in the south (40.03%) and Aymara in the north (35.61%) as expected from the historical location of these ethnic groups. We make our results available through an online app and demonstrate how it can be used to adjust for ancestry when testing association between incidence of a disease and nongenetic risk factors.ConclusionsWe have conducted the most extensive sampling, across many different cities, of current Chilean population. Ancestry varied significantly by latitude and human development. The panel of AIMs is available to the community for estimating ancestry at low cost in Chileans and other populations with similar ancestry.
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- 2020
15. The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) mission
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Olinto, A. V., Adams, J. H., Aloisio, R., Anchordoqui, L. A., Bergman, D. R., Bertaina, M. E., Bertone, P., Bisconti, F., Bustamante, M., Casolino, M., Christl, M. J., Cummings, A. L., De Mitri, I., Diesing, R., Eser, J. B., Fenu, F., Guépin, C., Hays, E. A., Judd, E., Krizmanic, J. F., Kuznetsov, E., Liberatore, A., Mackovjak, S., McEnery, J., Mitchell, J. W., Neronov, A., Oikonomou, F., Otte, A. N., Parizot, E., Paul, T. C., Perkins, J. S., Prévôt, G., Reardon, P., Reno, M. H., Ricci, M., Sarazin, F., Shinozaki, K., Soriano, J. F., Stecker, F., Takizawa, Y., Ulrich, R., Unger, M., Venters, T., Wiencke, L., and Young, R. M.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,High Energy Physics - Experiment - Abstract
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to observe cosmic neutrinos (CNs) above 20 PeV and ultra-high energy cosmic rays (UHECRs) above 20 EeV over the full sky. The POEMMA mission calls for two identical satellites flying in loose formation, each comprised of a 4-meter wide field-of-view (45 degrees) Schmidt photometer. The hybrid focal surface includes a fast (1 ${\mu}$s) ultraviolet camera for fluorescence observations and an ultrafast (10 ns) optical camera for Cherenkov observations. POEMMA will provide new multi-messenger windows onto the most energetic events in the universe, enabling the study of new astrophysics and particle physics at these otherwise inaccessible energies., Comment: 8 pages, 6 figures, presented in 36th International Cosmic Ray Conference (Madison). arXiv admin note: substantial text overlap with arXiv:1907.06217
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- 2019
16. POEMMA (Probe of Extreme Multi-Messenger Astrophysics) design
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Olinto, A. V., Adams, J. H., Aloisio, R., Anchordoqui, L. A., Bergman, D. R., Bertaina, M. E., Bertone, P., Bisconti, F., Bustamante, M., Casolino, M., Christl, M. J., Cummings, A. L., De Mitri, I., Diesing, R., Eser, J., Fenu, F., Guepin, C., Hays, E. A., Judd, E. G., Krizmanic, J. F., Kuznetsov, E., Liberatore, A., Mackovjak, S., McEnery, J., Mitchell, J. W., Neronov, A., Oikonomou, F., Otte, A. N., Parizot, E., Paul, T., Perkins, J. S., Prevot, G., Reardon, P., Reno, M. H., Ricci, M., Sarazin, F., Shinozaki, K., Soriano, J. F., Stecker, F., Takizawa, Y., Ulrich, R., Unger, M., Venters, T. M., Wiencke, L., and Young, R. M.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment - Abstract
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is a NASA Astrophysics probe-class mission designed to observe ultra-high energy cosmic rays (UHECRs) and cosmic neutrinos from space. Astro2020 APC white paper: Medium-class Space Particle Astrophysics Project., Comment: Astro2020 APC white paper: Medium-class Space Particle Astrophysics Project
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- 2019
17. Evaluating ocean health and restoration success: A comprehensive study of the benthic quality index in the Bilbao estuary
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Wawrzynkowski, P., Bustamante, M., Tajadura, F.J., and Becerro, M.A.
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- 2023
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18. 700,000 years of tropical Andean glaciation
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Rodbell, D. T., Hatfield, R. G., Abbott, M. B., Chen, C. Y., Woods, A., Stoner, J. S., McGee, D., Tapia, P. M., Bush, M., Valero-Garcés, B. L., Lehmann, S. B., Mark, S. Z., Weidhaas, N. C., Hillman, A. L., Larsen, D. J., Delgado, G., Katz, S. A., Solada, K. E., Morey, A. E., Finkenbinder, M., Valencia, B., Rozas-Davila, A., Wattrus, N., Colman, S. M., Bustamante, M. G., Kück, J., and Pierdominici, S.
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- 2022
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19. Snowmass white paper: beyond the standard model effects on neutrino flavor: Submitted to the proceedings of the US community study on the future of particle physics (Snowmass 2021)
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Argüelles, C. A., Barenboim, G., Bustamante, M., Coloma, P., Denton, P. B., Esteban, I., Farzan, Y., Martínez, E. Fernández, Forero, D. V., Gago, A. M., Katori, T., Lehnert, R., Ross-Lonergan, M., Suliga, A. M., Tabrizi, Z., Anchordoqui, L., Chakraborty, K., Conrad, J., Das, A., Fong, C. S., Littlejohn, B. R., Maltoni, M., Parno, D., Spitz, J., Tang, J., and Wissel, S.
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- 2023
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20. Banks’ Market Power, Access to Finance, and Leverage
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Bustamante, M Cecilia, primary and D’Acunto, Francesco, additional
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- 2024
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21. Comparative study on the load bearing capacity of driven steel H piles in a layered marl
- Author
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Bustamante, M., primary, Gianeselli, L., additional, and Schreiner, C., additional
- Published
- 2022
- Full Text
- View/download PDF
22. POEMMA: Probe Of Extreme Multi-Messenger Astrophysics
- Author
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Olinto, A. V., Adams, J. H., Aloisio, R., Anchordoqui, L. A., Bergman, D. R., Bertaina, M. E., Bertone, P., Bustamante, M., Christl, M. J., Csorna, S. E., Eser, J. B., Fenu, F., Guépin, C., Hays, E. A., Hunter, S., Judd, E., Jun, I., Kotera, K., Krizmanic, J. F., Kuznetsov, E., Mackovjak, S., Martinez-Sierra, L. M., Mastafa, M., Matthews, J. N., McEnery, J., Mitchell, J. W., Neronov, A., Otte, A. N., Parizot, E., Paul, T. C., Perkins, J. S., Prevot, G., Reardon, P., Reno, M. H., Sarazin, F., Shinozaki, K., Stecker, F., Streitmatter, R., Venters, T., Wiencke, L., and Young, R. M.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) mission is being designed to establish charged-particle astronomy with ultra-high energy cosmic rays (UHECRs) and to observe cosmogenic tau neutrinos (CTNs). The study of UHECRs and CTNs from space will yield orders-of-magnitude increase in statistics of observed UHECRs at the highest energies, and the observation of the cosmogenic flux of neutrinos for a range of UHECR models. These observations should solve the long-standing puzzle of the origin of the highest energy particles ever observed, providing a new window onto the most energetic environments and events in the Universe, while studying particle interactions well beyond accelerator energies. The discovery of CTNs will help solve the puzzle of the origin of UHECRs and begin a new field of Astroparticle Physics with the study of neutrino properties at ultra-high energies., Comment: 8 pages, in the Proceedings of the 35th International Cosmic Ray Conference, ICRC217, Busan, Korea
- Published
- 2017
23. Is it traction or pressure? Case series of hair system‐induced alopecia in six patients.
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Gil‐Redondo, R., Hermosa‐Gelbard, A., Saceda‐Corralo, D., Pindado‐Ortega, C., Porriño‐Bustamante, M. L., Jiménez‐Cauhé, J., and Vañó‐Galván, S.
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BALDNESS ,MESOTHERAPY ,PSYCHOLOGICAL factors ,TELEVISION viewing ,ALOPECIA areata ,SYMPTOMS - Abstract
This article presents a case series of hair system-induced alopecia in six Caucasian women. The patients experienced exacerbated hair loss in areas where the hair system was attached. Trichoscopy revealed features of both traction alopecia and pressure alopecia, suggesting a combined mechanism of action. The study highlights the need for dermatologists to be aware of this complication and familiar with trichoscopy to differentiate it from other conditions. However, the study has limitations, including a small sample size and lack of histopathological studies. [Extracted from the article]
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- 2024
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24. Terapia farmacológica en insuficiencia cardiaca fracción de eyección reducida: ¿cómo, cuánto, a quién?
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Cañete P., Iván, primary, De la Carrera V., Agustín, additional, Gil L., Antonia, additional, Orchard B., Ian, additional, Llancaqueo V., Marcelo, additional, and Bustamante M., Sergio, additional
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- 2024
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- View/download PDF
25. Introducing the Concept of Interaction Model for Interactive Dimensionality Reduction and Data Visualization
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Ortega-Bustamante, M. C., Hasperué, W., Peluffo-Ordóñez, D. H., Paéz-Jaime, M., Marrufo-Rodríguez, I., Rosero-Montalvo, P., Umaquinga-Criollo, A. C., Vélez-Falconi, M., Goos, Gerhard, Founding Editor, Hartmanis, Juris, Founding Editor, Bertino, Elisa, Editorial Board Member, Gao, Wen, Editorial Board Member, Steffen, Bernhard, Editorial Board Member, Woeginger, Gerhard, Editorial Board Member, Yung, Moti, Editorial Board Member, Gervasi, Osvaldo, editor, Murgante, Beniamino, editor, Misra, Sanjay, editor, Garau, Chiara, editor, Blečić, Ivan, editor, Taniar, David, editor, Apduhan, Bernady O., editor, Rocha, Ana Maria A.C., editor, Tarantino, Eufemia, editor, Torre, Carmelo Maria, editor, and Karaca, Yeliz, editor
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- 2020
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26. Unitary model for atomic ionization by intense XUV laser pulses
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Bustamante, M. G. and Rodríguez, V. D.
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Physics - Atomic Physics - Abstract
A unitary model describing the electronic transitions in an atom subject to a strong high frequency laser pulse is proposed. The model fully accounts for the initial state coupling with the continuum spectrum. Continuum-continuum as well as discrete-discrete transitions are neglected. The model leads to a single integro-differential equation for the initial state amplitude. Exact numerical and approximate closed semi-analytical solutions of this equation are obtained. A comparison of present results with full time dependent Schr\"odinger equation solution for Hydrogen atoms subject to a laser pulse is presented. The initial state time dependent population is rather well described by the model and two approximate solutions. The electron energy spectrum is also well reproduced by the model and by a new improved Weiskopf-Wigner related approximation., Comment: 9 pages, 5 figures
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- 2016
27. Constraints on the Ultra-High Energy Neutrino Flux from Gamma-Ray Bursts from a Prototype Station of the Askaryan Radio Array
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Allison, P., Auffenberg, J., Bard, R., Beatty, J. J., Besson, D. Z., Bora, C., Chen, C. -C., Chen, P., Connolly, A., Davies, J. P., DuVernois, M. A., Fox, B., Gorham, P. W., Hanson, K., Hill, B., Hoffman, K. D., Hong, E., Hu, L. -C., Ishihara, A., Karle, A., Kelley, J., Kravchenko, I., Landsman, H., Laundrie, A., Li, C. -J., Liu, T., Lu, M. -Y., Maunu, R., Mase, K., Meures, T., Miki, C., Nam, J., Nichol, R. J., Nir, G., O'Murchadha, A., Pfendner, C. G., Ratzlaff, K., Rotter, B., Sandstrom, P., Seckel, D., Shultz, A., Song, M., Stockham, J., Stockham, M., Sullivan, M., Touart, J., Tu, H. -Y., Varner, G. S., Yoshida, S., Young, R., Bustamante, M., and Guetta, D.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We report on a search for ultra-high-energy (UHE) neutrinos from gamma-ray bursts (GRBs) in the data set collected by the Testbed station of the Askaryan Radio Array (ARA) in 2011 and 2012. From 57 selected GRBs, we observed no events that survive our cuts, which is consistent with 0.12 expected background events. Using NeuCosmA as a numerical GRB reference emission model, we estimate upper limits on the prompt UHE GRB neutrino fluence and quasi-diffuse flux from $10^{7}$ to $10^{10}$ GeV. This is the first limit on the prompt UHE GRB neutrino quasi-diffuse flux above $10^{7}$ GeV., Comment: 14 pages, 8 figures, Published in Astroparticle Physics Journal
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- 2015
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28. Nanomaterials, Polymers, and Smart Packaging for Food Materials
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Marin-Bustamante, M. Q., Chanona-Pérez, J. J., Gϋemes-Vera, N., Mendoza-Pérez, J. A., Reséndiz-Mora, C. A., Cásarez-Santiago, R. G., Rojas-Candelas, L. E., and Prasad, Ram, Series Editor
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- 2019
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29. Nanoagriculture and Energy Advances
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Cásarez-Santiago, R. G., Chanona-Pérez, J. J., Reséndiz-Mora, C. A., Gϋemes-Vera, N., Manzo-Robledo, A., Perea-Flores, M. J., Marin-Bustamante, M. Q., and Prasad, Ram, Series Editor
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- 2019
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30. Protocolo de prevención y vigilancia endoscópica de la displasia/cáncer colorrectal en la enfermedad inflamatoria intestinal
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Nos, P., Bustamante, M., Pellisé, M., and Clofent, J.
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- 2020
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31. The Milky Way shines in high-energy neutrinos
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Bustamante, M., primary
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- 2023
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32. First Report of Phyllactinia chubutiana Causing Powdery Mildew on Goji Berry Plants (Lycium barbarum and L. chinense) in the United States
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Elfar, K., primary, Bustamante, M. I., additional, Rooney-Latham, S., additional, Eskalen, A., additional, and Miller, T., additional
- Published
- 2023
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- View/download PDF
33. HPR103 Potential Impacts of the EMA-HMA Join Statement Supporting Biosimilar Interchangeability in Biosimilar Access in the EU
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Ribeiro, A., primary, Sazakli, E.A., additional, O'Hara, M., additional, and Martin De Bustamante, M., additional
- Published
- 2023
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34. HTA218 Public Engagement and Its Influence on Health Technology Assessment Outcomes in Latin America
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Tôrres, L., primary, Nacazume, J., additional, Vega, M., additional, Boers Trilles, V., additional, Bustamante, M., additional, and Ribeiro, A., additional
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- 2023
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35. Measurement of muon plus proton final states in $\nu_{\mu}$ Interactions on Hydrocarbon at $\langle$$E_{\nu}$$\rangle$ = 4.2 GeV
- Author
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Walton, T., Betancourt, M., Aliaga, L., Altinok, O., Bodek, A., Bravar, A., Budd, H., Bustamante, M. J., Butkevich, A., Caicedo, D. A. Martinez, Carneiro, M. F., Castromonte, C. M., Christy, M. E., Chvojka, J., da Motta, H., Datta, M., Devan, J., Dytman, S. A., Díaz, G. A., Eberly, B., Felix, J., Fields, L., Fine, R., Fiorentini, G. A., Gago, A. M., Gallagher, H., Gran, R., Harris, D. A., Higuera, A., Hurtado, K., Kleykamp, J., Kordosky, M., Kulagin, S. A., Le, T., Maher, E., Manly, S., Mann, W. A., Marshall, C. M., Mari, C. Martin, McFarland, K. S., McGivern, C. L., McGowan, A. M., Messerly, B., Miller, J., Mislivec, A., Morfín, J. G., Mousseau, J., Muhlbeier, T., Naples, D., Nelson, J. K., Norrick, A., Osta, J., Paolone, V., Park, J., Patrick, C. E., Perdue, G. N., Rakotondravohitra, L., Ransome, R. D., Ray, H., Ren, L., Rodrigues, P. A., Ruterbories, D., Schellman, H., Schmitz, D. W., Simon, C., Snider, F. D., Sobczyk, J. T., Salinas, C. J. Solano, Tagg, N., Tice, B. G., Valencia, E., Wolcott, J., Wospakrik, M., Zavala, G., Zhang, D., and Ziemer, B. P.
- Subjects
High Energy Physics - Experiment - Abstract
A study of charged-current muon neutrino scattering on hydrocarbon in which the final state includes a muon and a proton and no pions is presented. Although this signature has the topology of neutrino quasielastic scattering from neutrons, the event sample contains contributions from both quasielastic and inelastic processes where pions are absorbed in the nucleus. The analysis accepts events with muon production angles up to 70$^{\circ}$ and proton kinetic energies greater than 110 MeV. The extracted cross section, when based completely on hadronic kinematics, is well-described by a simple relativistic Fermi gas nuclear model including the neutrino event generator modeling for inelastic processes and particle transportation through the nucleus. This is in contrast to the quasielastic cross section based on muon kinematics, which is best described by an extended model that incorporates multi-nucleon correlations. This measurement guides the formulation of a complete description of neutrino-nucleus interactions that encompasses the hadronic as well as the leptonic aspects of this process., Comment: total 10 pages, 5 figures, 2 pages of supplemental materials. Published in Physical Review D (Rapid Communication) April 1, 2015
- Published
- 2014
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36. Genotype Prevalence of Lactose Deficiency, Vitamin D Deficiency, and the Vitamin D Receptor in a Chilean Inflammatory Bowel Disease Cohort: Insights from an Observational Study
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Pérez-Jeldres, Tamara, primary, Bustamante, M. Leonor, additional, Segovia-Melero, Roberto, additional, Aguilar, Nataly, additional, Magne, Fabien, additional, Ascui, Gabriel, additional, Uribe, Denisse, additional, Azócar, Lorena, additional, Hernández-Rocha, Cristián, additional, Estela, Ricardo, additional, Silva, Verónica, additional, De La Vega, Andrés, additional, Arriagada, Elizabeth, additional, Gonzalez, Mauricio, additional, Onetto, Gian-Franco, additional, Escobar, Sergio, additional, Baez, Pablo, additional, Zazueta, Alejandra, additional, Pavez-Ovalle, Carolina, additional, Miquel, Juan Francisco, additional, and Álvarez-Lobos, Manuel, additional
- Published
- 2023
- Full Text
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37. Charged Pion Production in $\nu_\mu$ Interactions on Hydrocarbon at $\langle E_{\nu}\rangle$= 4.0 GeV
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Eberly, B., Aliaga, L., Altinok, O., Sazo, M. G. Barrios, Bellantoni, L., Betancourt, M., Bodek, A., Bravar, A., Budd, H., Bustamante, M. J., Butkevich, A., Caicedo, D. A. Martinez, Carneiro, M. F., Christy, M. E., Chvojka, J., da Motta, H., Datta, M., Devan, J., Dytman, S. A., Díaz, G. A., Felix, J., Fields, L., Fine, R., Fiorentini, G. A., Gago, A. M., Galindo, R., Gallagher, H., Golan, T., Gran, R., Harris, D. A., Higuera, A., Hurtado, K., Kafka, T., Kleykamp, J., Kordosky, M., Le, T., Maher, E., Manly, S., Mann, W. A., Marshall, C. M., McFarland, K. S., McGivern, C. L., McGowan, A. M., Messerly, B., Miller, J., Mislivec, A., Morfín, J. G., Mousseau, J., Muhlbeier, T., Naples, D., Nelson, J. K., Norrick, A., Osta, J., Palomino, J. L., Paolone, V., Park, J., Patrick, C. E., Perdue, G. N., Rakotondravohitra, L., Ramirez, M. A., Ransome, R. D., Ray, H., Ren, L., Rodrigues, P. A., Ruterbories, D., Salazar, G., Schellman, H., Schmitz, D. W., Simon, C., Sobczyk, J. T., Salinas, C. J. Solano, Tagg, N., Tice, B. G., Valencia, E., Walton, T., Wolcott, J., Wospakrik, M., Zavala, G., Zegarra, A., Zhang, D., and Ziemer, B. P.
- Subjects
High Energy Physics - Experiment - Abstract
Charged pion production via charged current $\nu_{\mu}$ interactions on plastic (CH) is studied using the MINERvA detector exposed to the NuMI wideband neutrino beam at Fermilab. Events with hadronic invariant mass W $<$ 1.4 GeV are selected to isolate single pion production, which is expected to occur primarily through the $\Delta(1232)$ resonance. Cross sections as functions of pion production angle and kinetic energy are reported and compared to predictions from different theoretical calculations and generator-based models, for neutrinos ranging in energy from 1.5 GeV to 10 GeV. The data are best described by calculations which include significant contributions from pion intranuclear rescattering. These measurements constrain the primary interaction rate and the role of final state interactions in pion production, both of which need to be well understood by neutrino oscillation experiments., Comment: 23 pages, 13 figures. Submitted to Physical Review D
- Published
- 2014
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38. Measurement of Ratios of $\nu_{\mu}$ Charged-Current Cross Sections on C, Fe, and Pb to CH at Neutrino Energies 2-20 GeV
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Tice, B. G., Datta, M., Mousseau, J., Aliaga, L., Altinok, O., Sazo, M. G. Barrios, Betancourt, M., Bodek, A., Bravar, A., Brooks, W. K., Budd, H., Bustamante, M. J., Butkevich, A., Caicedo, D. A. Martinez, Castromonte, C. M., Christy, M. E., Chvojka, J., da Motta, H., Devan, J., Dytman, S. A., Díaz, G. A., Eberly, B., Felix, J., Fields, L., Fiorentini, G. A., Gago, A. M., Gallagher, H., Gran, R., Harris, D. A., Higuera, A., Hurtado, K., Jerkins, M., Kafka, T., Kordosky, M., Kulagin, S. A., Le, T., Maggi, G., Maher, E., Manly, S., Mann, W. A., Marshall, C. M., Mari, C. Martin, McFarland, K. S., McGivern, C. L., McGowan, A. M., Miller, J., Mislivec, A., Morfín, J. G., Muhlbeier, T., Naples, D., Nelson, J. K., Norrick, A., Osta, J., Palomino, J. L., Paolone, V., Park, J., Patrick, C. E., Perdue, G. N., Rakotondravohitra, L., Ransome, R. D., Ray, H., Ren, L., Rodrigues, P. A., Savage, D. G., Schellman, H., Schmitz, D. W., Simon, C., Snider, F. D., Salinas, C. J. Solano, Tagg, N., Valencia, E., Velásquez, J. P., Walton, T., Wolcott, J., Zavala, G., Zhang, D., and Ziemer, B. P.
- Subjects
High Energy Physics - Experiment ,Nuclear Experiment - Abstract
We present measurements of $\nu_{\mu}$ charged-current cross section ratios on carbon, iron, and lead relative to a scintillator (CH) using the fine-grained MINERvA detector exposed to the NuMI neutrino beam at Fermilab. The measurements utilize events of energies $2
=8~GeV$, which have a reconstructed $\mu^{-}$ scattering angle less than $17^\circ$ to extract ratios of inclusive total cross sections as a function of neutrino energy $E_{\nu}$ and flux-integrated differential cross sections with respect to the Bjorken scaling variable $x$. These results provide the first high-statistics direct measurements of nuclear effects in neutrino scattering using different targets in the same neutrino beam. Measured cross section ratios exhibit a relative depletion at low $x$ and enhancement at large $x$. Both become more pronounced as the nucleon number of the target nucleus increases. The data are not reproduced by GENIE, a conventional neutrino-nucleus scattering simulation, or by the alternative models for the nuclear dependence of inelastic scattering that are considered., Comment: 6 pages, 2 figures, 7 pages of supplemental material. Published in Physical Review Letters June 13, 2014 - Published
- 2014
- Full Text
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39. Validation of a Football Helmet Finite Element Model and Quantification of Impact Energy Distribution
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Corrales, M. A., Gierczycka, D., Barker, J., Bruneau, D., Bustamante, M. C., and Cronin, D. S.
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- 2020
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40. Experimental Testing and Computational Analysis of Viscoelastic Wave Propagation in Polymeric Split Hopkinson Pressure Bar
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Bustamante, M., Cronin, D. S., Singh, D., Zimmerman, Kristin B., Series editor, Kimberley, Jamie, editor, Lamberson, Leslie, editor, and Mates, Steven, editor
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- 2018
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41. Ideal evolution of MHD turbulence when imposing Taylor-Green symmetries
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Brachet, M. E., Bustamante, M. D., Krstulovic, G., Mininni, P. D., Pouquet, A., and Rosenberg, D.
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Physics - Plasma Physics ,Mathematical Physics ,Physics - Fluid Dynamics - Abstract
We investigate the ideal and incompressible magnetohydrodynamic (MHD) equations in three space dimensions for the development of potentially singular structures. The methodology consists in implementing the four-fold symmetries of the Taylor-Green vortex generalized to MHD, leading to substantial computer time and memory savings at a given resolution; we also use a re-gridding method that allows for lower-resolution runs at early times, with no loss of spectral accuracy. One magnetic configuration is examined at an equivalent resolution of $6144^3$ points, and three different configurations on grids of $4096^3$ points. At the highest resolution, two different current and vorticity sheet systems are found to collide, producing two successive accelerations in the development of small scales. At the latest time, a convergence of magnetic field lines to the location of maximum current is probably leading locally to a strong bending and directional variability of such lines. A novel analytical method, based on sharp analysis inequalities, is used to assess the validity of the finite-time singularity scenario. This method allows one to rule out spurious singularities by evaluating the rate at which the logarithmic decrement of the analyticity-strip method goes to zero. The result is that the finite-time singularity scenario cannot be ruled out, and the singularity time could be somewhere between $t=2.33$ and $t=2.70.$ More robust conclusions will require higher resolution runs and grid-point interpolation measurements of maximum current and vorticity., Comment: 18 pages, 13 figures, 2 tables; submitted to Physical Review E
- Published
- 2012
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42. Design of axially loaded piles — French practice
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Bustamante, M., primary and Frank, R., additional
- Published
- 2020
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43. SUSY Renormalization Group Effects in Ultra High Energy Neutrinos
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Bustamante, M., Gago, A. M., and Jones-Perez, J.
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High Energy Physics - Phenomenology ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We have explored the question of whether the renormalization group running of the neutrino mixing parameters in the Minimal Supersymmetric Standard Model is detectable with ultra-high energy neutrinos from active galactic nuclei (AGN). We use as observables the ratios of neutrino fluxes produced at the AGN, focusing on four different neutrino production models: $(\Phi_{\nu_e+\bar{\nu}_e}^0 : \Phi_{\nu_\mu+\bar{\nu}_\mu}^0 : \Phi_{\nu_\tau+\bar{\nu}_\tau}^0)$ = (1:2:0), (0:1:0), (1:0:0), and (1:1:0). The prospects for observing deviations experimentally are taken into consideration, and we find out that it is necessary to impose a cut-off on the transferred momentum of $Q^2 \geq 10^7$ GeV$^2$. However, this condition, together with the expected low value of the diffuse AGN neutrino flux, yields a negligible event rate at a km-scale Cherenkov detector such as IceCube., Comment: 26 pages, 9 figures. Version accepted for publication in JHEP
- Published
- 2010
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44. IceCube expectations for two high-energy neutrino production models at active galactic nuclei
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Argüelles, C. A., Bustamante, M., and Gago, A. M.
- Subjects
Astrophysics - High Energy Astrophysical Phenomena ,High Energy Physics - Phenomenology - Abstract
We have determined the currently allowed regions of the parameter spaces of two representative models of diffuse neutrino flux from active galactic nuclei (AGN): one by Koers & Tinyakov (KT) and another by Becker & Biermann (BB). Our observable has been the number of upgoing muon-neutrinos expected in the 86-string IceCube detector, after 5 years of exposure, in the range 10^5 < E/GeV < 10^8. We have used the latest estimated discovery potential of the IceCube-86 array at the 5-sigma level to determine the lower boundary of the regions, while for the upper boundary we have used either the AMANDA upper bound on the neutrino flux or the more recent preliminary upper bound given by the half-completed IceCube-40 array (IC40). We have varied the spectral index of the proposed power-law fluxes, alpha, and two parameters of the BB model: the ratio between the boost factors of neutrinos and cosmic rays, Gamma_nu/Gamma_{CR}, and the maximum redshift of the sources that contribute to the cosmic-ray flux, zCRmax. For the KT model, we have considered two scenarios: one in which the number density of AGN does not evolve with redshift and another in which it evolves strongly, following the star formation rate. Using the IC40 upper bound, we have found that the models are visible in IceCube-86 only inside very thin strips of parameter space and that both of them are discarded at the preferred value of alpha = 2.7 obtained from fits to cosmic-ray data. Lower values of alpha, notably the values 2.0 and 2.3 proposed in the literature, fare better. In addition, we have analysed the capacity of IceCube-86 to discriminate between the models within the small regions of parameter space where both of them give testable predictions. Within these regions, discrimination at the 5-sigma level or more is guaranteed., Comment: 24 pages, 6 figures, v2: new IceCube-40 astrophysical neutrino upper bound and IceCube-86 discovery potential used, explanation of AGN flux models improved, only upgoing neutrinos used, conclusions strengthened. Accepted for publication in JCAP
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- 2010
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45. Energy-independent new physics in the flavour ratios of high-energy astrophysical neutrinos
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Bustamante, M., Gago, A. M., and Pena-Garay, C.
- Subjects
High Energy Physics - Phenomenology - Abstract
We have studied the consequences of breaking the CPT symmetry in the neutrino sector, using the expected high-energy neutrino flux from distant cosmological sources such as active galaxies. For this purpose we have assumed three different hypotheses for the neutrino production model, characterised by the flavour fluxes at production \phi_e^0:\phi_\mu^0:\phi_\tau^0 = 1:2:0, 0:1:0, and 1:0:0, and studied the theoretical and experimental expectations for the muon-neutrino flux at Earth, \phi_\mu, and for the flavour ratios at Earth, R = \phi_\mu/\phi_e and S = \phi_\tau/\phi_\mu. CPT violation (CPTV) has been implemented by adding an energy-independent term to the standard neutrino oscillation Hamiltonian. This introduces three new mixing angles, two new eigenvalues and three new phases, all of which have currently unknown values. We have varied the new mixing angles and eigenvalues within certain bounds, together with the parameters associated to pure standard oscillations. Our results indicate that, for the models 1:2:0 and 0:1:0, it might possible to find large deviations for \phi_\mu, R, and S between the cases without and with CPTV, provided the CPTV eigenvalues lie within 10^{-29}-10^{-27} GeV, or above. Moreover, if CPTV exists, there are certain values of R and S that can be accounted for by up to three production models. If no CPTV were observed, we could set limits on the CPTV eigenvalues of the same order. Detection prospects calculated using IceCube suggest that for the models 1:2:0 and 0:1:0, the modifications due to CPTV are larger and more clearly separable from the standard-oscillations predictions. We conclude that IceCube is potentially able to detect CPTV but that, depending on the values of the CPTV parameters, there could be a mis-determination of the neutrino production model., Comment: 28 pages, 8 figures. Fixes number of nucleon targets in ice and Figure 8. More legible figures. Bibliography expanded. Matches version accepted for publication in JHEP.
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- 2010
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46. Beyond the Standard Model for Montaneros
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Bustamante, M., Cieri, L., and Ellis, John
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High Energy Physics - Phenomenology - Abstract
These notes cover (i) electroweak symmetry breaking in the Standard Model (SM) and the Higgs boson, (ii) alternatives to the SM Higgs boson including an introduction to composite Higgs models and Higgsless models that invoke extra dimensions, (iii) the theory and phenomenology of supersymmetry, and (iv) various further beyond topics, including Grand Unification, proton decay and neutrino masses, supergravity, superstrings and extra dimensions., Comment: Based on lectures by John Ellis at the 5th CERN-Latin-American School of High-Energy Physics, Recinto Quirama, Colombia, 15 - 28 Mar 2009, 84 pages, 35 figures
- Published
- 2009
47. High energy astrophysical neutrino flux and modified dispersion relations
- Author
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Alba, J. L. Bazo, Bustamante, M., Gago, A. M., and Miranda, O. G.
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High Energy Physics - Phenomenology - Abstract
Motivated by the interest in searches for violation of CPT invariance, we study its possible effects in the flavour ratios of high-energy neutrinos coming from cosmic accelerators. In particular, we focus on the effect of an energy independent new physics contribution to the neutrino flavour oscillation phase and explore whether it is observable in future detectors. Such a contribution could be related not only to CPT violation but also to a nonuniversal coupling of neutrinos to a torsion field. We conclude that this extra phase contribution only becomes observable, in the best case, at energies greater than 10^{16.5} GeV, which is about five orders of magnitude higher than the most energetic cosmological neutrinos to be detected in the near future. Therefore, if these effects are present only in the oscillation phase, they are going to be unobservable, unless a new mechanism or source capable to produce neutrinos of such energy were detected., Comment: Accepted for publication in the Int. J. Mod. Phys. A -- Typo in online version of abstract corrected
- Published
- 2009
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48. Extreme scenarios of new physics in the UHE astrophysical neutrino flavour ratios
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Bustamante, M., Gago, A. M., and Pena-Garay, C.
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High Energy Physics - Phenomenology - Abstract
We add an energy-independent Hamiltonian to the standard flavour oscillation one. This kind of physics might appear in theories where neutrinos couple differently to a plausible non-zero torsion of the gravitational field or more dramatically in the presence of CPT-violating physics in the flavour oscillations. If this contribution exists, experiments at higher energies are more sensitive to their free parameters, and flavour conversion could be severely modified. We show that this new physics modifies the neutrino mixing angles and find expressions that relate the new, effective, angles to the standard oscillation parameters \Delta_m_{ij}^2, \theta_{ij} and \delta_{CP}, and to the parameters in the new-physics Hamiltonian, within a three-neutrino formalism. We consider scenarios where the new parameters allow for extreme deviations of the expected neutrino flavour ratios at Earth from their standard values. We show that large departures of the standard flavour scenario are plausible, which would be a strong hint of the violation of a conserved symmetry., Comment: 10 pages, To appear in the proceedings of DISCRETE'08: Symposium on Prospects in the Physics of Discrete Symmetries, Valencia, Spain, 11-16 Dec 2008
- Published
- 2009
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49. Seguridad de minoxidil oral a dosis bajas en pacientes con hipertensión o arritmias: estudio multicéntrico de 264 pacientes
- Author
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Cauhe, J Jimenez, primary, Pirmez, R, additional, Ramos, P Müller, additional, Melo, D Fernandes, additional, Quijano, D Ortega, additional, Moreno-Arrones, O M, additional, Corralo, D Saceda, additional, Redondo, R Gil, additional, Gelbard, A Hermosa, additional, Sanabria, B Dias, additional, Restom, D, additional, Porriño-Bustamante, M L, additional, Ortega, C Pindado, additional, Rico, E Berna, additional, Nieto, D Fernandez, additional, Ramos, M, additional, Olasolo, P Jaen, additional, and Galvan, S Vaño, additional
- Published
- 2023
- Full Text
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50. First Report of Neofusicoccum mediterraneum and Neofusicoccum parvum Causing Pine Ghost Canker on Pinus spp. in Southern California
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Bustamante, M. I., primary, Lynch, S. C., additional, Elfar, K., additional, Kabashima, J., additional, Wood, R., additional, Neault, H. F., additional, Rauhe, M. B., additional, Crain, J., additional, Lopez, J. A., additional, Penicks, A., additional, Mojica, H., additional, Atkinson, M. D., additional, Shogren, C., additional, Arreguin, M., additional, Chiang, C. F., additional, Wells, S. I., additional, Alarcon, K. S., additional, and Eskalen, A., additional
- Published
- 2023
- Full Text
- View/download PDF
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