# NuOscProbExact: a general-purpose code to compute exact two-flavor and three-flavor neutrino oscillation probabilities

- Published: 28 Apr 2019

- Niels Bohr Institute Denmark

mbustamante@nbi.ku.dk; ORCID: 0000-0001-6923-

0865 [1] B. Pontecorvo, Sov. Phys. JETP 26, 984 (1968), [Zh.

Eksp. Teor. Fiz. 53, 1717 (1967)]. [2] V. D. Barger, K. Whisnant, and R. J. N. Phillips, Phys.

Rev. D 22, 1636 (1980). [3] S. M. Bilenky, Proc. Roy. Soc. Lond. A 460, 403 (2004). [4] G. Fantini, A. Gallo Rosso, F. Vissani, and V. Zema,

Adv. Ser. Direct. High Energy Phys. 28, 37 (2018),

arXiv:1802.05781 [hep-ph]. [5] T. Kajita, Rev. Mod. Phys. 88, 030501 (2016). [6] A. B. McDonald, Rev. Mod. Phys. 88, 030502 (2016). [7] B. Kayser, Phys. Rev. D 24, 110 (1981). [8] C. Giunti and C. W. Kim, Fundamentals of Neutrino

Physics and Astrophysics (2007). [9] M. Tanabashi et al. (Particle Data Group), Phys. Rev.

D 98, 030001 (2018). [10] V. D. Barger, K. Whisnant, S. Pakvasa, and R. J. N.

Phillips, Phys. Rev. D 22, 2718 (1980), [, 300 (1980)]. [11] S. T. Petcov, Phys. Lett. B 200, 373 (1988). [12] H. W. Zaglauer and K. H. Schwarzer, Z. Phys. C 40,

273 (1988). [13] E. Torrente Lujan, Phys. Rev. D 53, 4030 (1996),

arXiv:hep-ph/9505209 [hep-ph]. [14] A. B. Balantekin, Phys. Rev. D 58, 013001 (1998),

arXiv:hep-ph/9712304 [hep-ph]. [15] S. R. Coleman and S. L. Glashow, Phys. Rev. D 59,

116008 (1999), arXiv:hep-ph/9812418 [hep-ph]. [16] A. M. Gago, M. M. Guzzo, H. Nunokawa, W. J. C.

Teves, and R. Zukanovich Funchal, Phys. Rev. D 64,

073003 (2001), arXiv:hep-ph/0105196 [hep-ph]. [17] K. Kimura, A. Takamura, and H. Yokomakura, Phys.

###### Related research

- Niels Bohr Institute Denmark

mbustamante@nbi.ku.dk; ORCID: 0000-0001-6923-

0865 [1] B. Pontecorvo, Sov. Phys. JETP 26, 984 (1968), [Zh.

Eksp. Teor. Fiz. 53, 1717 (1967)]. [2] V. D. Barger, K. Whisnant, and R. J. N. Phillips, Phys.

Rev. D 22, 1636 (1980). [3] S. M. Bilenky, Proc. Roy. Soc. Lond. A 460, 403 (2004). [4] G. Fantini, A. Gallo Rosso, F. Vissani, and V. Zema,

Adv. Ser. Direct. High Energy Phys. 28, 37 (2018),

arXiv:1802.05781 [hep-ph]. [5] T. Kajita, Rev. Mod. Phys. 88, 030501 (2016). [6] A. B. McDonald, Rev. Mod. Phys. 88, 030502 (2016). [7] B. Kayser, Phys. Rev. D 24, 110 (1981). [8] C. Giunti and C. W. Kim, Fundamentals of Neutrino

Physics and Astrophysics (2007). [9] M. Tanabashi et al. (Particle Data Group), Phys. Rev.

D 98, 030001 (2018). [10] V. D. Barger, K. Whisnant, S. Pakvasa, and R. J. N.

Phillips, Phys. Rev. D 22, 2718 (1980), [, 300 (1980)]. [11] S. T. Petcov, Phys. Lett. B 200, 373 (1988). [12] H. W. Zaglauer and K. H. Schwarzer, Z. Phys. C 40,

273 (1988). [13] E. Torrente Lujan, Phys. Rev. D 53, 4030 (1996),

arXiv:hep-ph/9505209 [hep-ph]. [14] A. B. Balantekin, Phys. Rev. D 58, 013001 (1998),

arXiv:hep-ph/9712304 [hep-ph]. [15] S. R. Coleman and S. L. Glashow, Phys. Rev. D 59,

116008 (1999), arXiv:hep-ph/9812418 [hep-ph]. [16] A. M. Gago, M. M. Guzzo, H. Nunokawa, W. J. C.

Teves, and R. Zukanovich Funchal, Phys. Rev. D 64,

073003 (2001), arXiv:hep-ph/0105196 [hep-ph]. [17] K. Kimura, A. Takamura, and H. Yokomakura, Phys.