Why 'ksi'(1690) and 'ksi'(2120) are so narrow? (2016)
- Authors:
- USP affiliated authors: NIELSEN, MARINA - IF ; TORRES, ALBERTO MARTINEZ - IF ; NAVARRA, FERNANDO SILVEIRA - IF
- Unidade: IF
- Subjects: CROMODINÂMICA QUÂNTICA; QUARK
- Language: Inglês
- Imprenta:
-
ABNT
KHEMCHANDANI, K. P. et al. Why 'ksi'(1690) and 'ksi'(2120) are so narrow?. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/1608.07086.pdf. Acesso em: 24 abr. 2024. , 2016 -
APA
Khemchandani, K. P., Hosaka, A., Nagahiro, H., Nielsen, M., Torres, A. M., & Navarra, F. S. (2016). Why 'ksi'(1690) and 'ksi'(2120) are so narrow? São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/1608.07086.pdf -
NLM
Khemchandani KP, Hosaka A, Nagahiro H, Nielsen M, Torres AM, Navarra FS. Why 'ksi'(1690) and 'ksi'(2120) are so narrow? [Internet]. 2016 ;[citado 2024 abr. 24 ] Available from: https://arxiv.org/pdf/1608.07086.pdf -
Vancouver
Khemchandani KP, Hosaka A, Nagahiro H, Nielsen M, Torres AM, Navarra FS. Why 'ksi'(1690) and 'ksi'(2120) are so narrow? [Internet]. 2016 ;[citado 2024 abr. 24 ] Available from: https://arxiv.org/pdf/1608.07086.pdf - Understanding close-lying exotic charmonia states within QCD sum rules
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- Update on J / 'psi' regeneration in a hadron gas
- On the absorption and production cross sections of 'K' and 'K' POT. *'
- Production and absorption of exotic bottomonium-like states in high energy heavy ion collisions
- X, Y and Z States
- Understanding close-lying exotic charmonia states within QCD sum rules
- Study of the 'D POT. *' 'rô' system using QCD sum rules
- X(3872) production and absorption in a hot hadron gas
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