Draft:Cervantes Wu

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Cervantes Wu
Born30.10.2006
Alma materStanford University
Known forTheoretical Physics
Scientific career
FieldsQuantum Physics, Particle Physics, Theoretical Physics
InstitutionsPrinceton University, IceCube Neutrino Observatory, Stanford University, New York University Game Center
Websitehttps://www.mriwu.us

Cervantes Wu, also known as Lum, is a person with interests in both the art and science fields. He has experience in game character design and has also participated in academic research related to quantum physics and particle physics.

Background[edit]

Wu's background includes participation in research projects at institutions such as Princeton University and IceCube Neutrino Observatory. He studied for his bachelor's degree at Stanford University[1][2].[3][4]

Artistic Activities[edit]

Wu works in game character design, creating characters with unique narratives and incorporating various stylistic influences.[5][6][7]

Scientific Contributions[edit]

Wu has contributed to research work in quantum physics and particle physics, and his work is documented in academic publications[8][9][10][11][12][13].[14][15]

References[edit]

  1. ^ "Cervantes Wu". sites.google.com. Retrieved 2024-04-22.
  2. ^ Wu, Cervantes. "Cervantes Wu's Stanford Alumni Directory".
  3. ^ Wu, Cervantes. "Cervantes Wu's LinkedIn profile".
  4. ^ "Cervantes Wu". scholar.google.com. Retrieved 2024-04-22.
  5. ^ "LUM (@MRiwu_u) / X". www.google.com. Retrieved 2024-04-22.
  6. ^ "LUM (@MRiwu_u) / X". www.google.com. Retrieved 2024-04-22.
  7. ^ "pixiv's High Schoolers Illustration Contest 2023 Results - From 1310 entries, the most ever, the winners are...?!". pixivision. 2023-10-14. Retrieved 2024-04-22.
  8. ^ Abbasi, Rasha; Ackermann, M.; Adams, J.; Agarwalla, S. K.; Aggarwal, N.; Aguilar, J. A.; Ahlers, M.; Alameddine, J. M.; Amin, N. M.; Andeen, K. (2023). "Limits on Neutrino Emission from GRB 221009A from MeV to PeV Using the IceCube Neutrino Observatory". The Astrophysical Journal Letters. 946 (1): L26. arXiv:2302.05459. Bibcode:2023ApJ...946L..26A. doi:10.3847/2041-8213/acc077.
  9. ^ Abbasi, R.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alispach, C.; Alves, A. A.; Amin, N. M.; An, R.; Andeen, K.; Anderson, T.; Anton, G.; Argüelles, C.; Ashida, Y. (2022-02-02). "Search for Relativistic Magnetic Monopoles with Eight Years of IceCube Data". Physical Review Letters. 128 (5): 051101. arXiv:2109.13719. Bibcode:2022PhRvL.128e1101A. doi:10.1103/PhysRevLett.128.051101. ISSN 0031-9007. PMID 35179913.
  10. ^ Abbasi, R.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alameddine, J. M.; Alispach, C.; Alves, A. A.; Amin, N. M.; Andeen, K.; Anderson, T.; Anton, G.; Argüelles, C.; Ashida, Y. (2022-07-22). "Search for neutrino emission from cores of active galactic nuclei". Physical Review D. 106 (2): 022005. arXiv:2111.10169. Bibcode:2022PhRvD.106b2005A. doi:10.1103/PhysRevD.106.022005. ISSN 2470-0010.
  11. ^ Abbasi, R.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alameddine, J. M.; Alispach, C.; Alves, A. A.; Amin, N. M.; Andeen, K.; Anderson, T.; Anton, G.; Argüelles, C.; Ashida, Y. (2022-03-21). "Search for GeV-scale dark matter annihilation in the Sun with IceCube DeepCore". Physical Review D. 105 (6): 062004. arXiv:2111.09970. Bibcode:2022PhRvD.105f2004A. doi:10.1103/PhysRevD.105.062004. ISSN 2470-0010.
  12. ^ Abbasi, Rasha; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alameddine, J. M.; Alves, A. A.; Amin, N. M.; Andeen, K. (2022). "Searches for neutrinos from gamma-ray bursts using the IceCube Neutrino Observatory". The Astrophysical Journal. 939 (2): 116. arXiv:2205.11410. Bibcode:2022ApJ...939..116A. doi:10.3847/1538-4357/ac9785.
  13. ^ IceCube Collaboration*†; Abbasi, R.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alameddine, J. M.; Alves, A. A.; Amin, N. M.; Andeen, K.; Anderson, T.; Anton, G.; Argüelles, C.; Ashida, Y. (2023-06-30). "Observation of high-energy neutrinos from the Galactic plane". Science. 380 (6652): 1338–1343. doi:10.1126/science.adc9818. ISSN 0036-8075. PMID 37384687.
  14. ^ Abbasi, Rasha; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alameddine, J. M.; Alispach, C.; Alves Jr, A. A.; Amin, N. M. (2022). "Improved characterization of the astrophysical muon–neutrino flux with 9.5 years of IceCube data". The Astrophysical Journal. 928 (1): 50. arXiv:2111.10299. Bibcode:2022ApJ...928...50A. doi:10.3847/1538-4357/ac4d29.
  15. ^ IceCube Collaboration*†; Abbasi, R.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alameddine, J. M.; Alispach, C.; Alves, A. A.; Amin, N. M.; Andeen, K.; Anderson, T.; Anton, G.; Argüelles, C. (2022-11-04). "Evidence for neutrino emission from the nearby active galaxy NGC 1068". Science. 378 (6619): 538–543. arXiv:2211.09972. Bibcode:2022Sci...378..538I. doi:10.1126/science.abg3395. ISSN 0036-8075. PMID 36378962.