Understanding the properties of 'ksi'(1690) and 'ksi'(2120) (2017)
- Authors:
- USP affiliated authors: TORRES, ALBERTO MARTINEZ - IF ; NAVARRA, FERNANDO SILVEIRA - IF ; NIELSEN, MARINA - IF
- Unidade: IF
- Subjects: CROMODINÂMICA QUÂNTICA; COLISÕES DE ÍONS PESADOS RELATIVÍSTICOS
- Language: Inglês
- Imprenta:
-
ABNT
KHEMCHANDANI, K. P. et al. Understanding the properties of 'ksi'(1690) and 'ksi'(2120). . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/abs/1712.09465. Acesso em: 19 set. 2024. , 2017 -
APA
Khemchandani, K. P., Hosakac, A., Nagahiro, H., Torres, A. M., Navarra, F. S., & Nielsen, M. (2017). Understanding the properties of 'ksi'(1690) and 'ksi'(2120). São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/abs/1712.09465 -
NLM
Khemchandani KP, Hosakac A, Nagahiro H, Torres AM, Navarra FS, Nielsen M. Understanding the properties of 'ksi'(1690) and 'ksi'(2120) [Internet]. 2017 ;[citado 2024 set. 19 ] Available from: https://arxiv.org/abs/1712.09465 -
Vancouver
Khemchandani KP, Hosakac A, Nagahiro H, Torres AM, Navarra FS, Nielsen M. Understanding the properties of 'ksi'(1690) and 'ksi'(2120) [Internet]. 2017 ;[citado 2024 set. 19 ] Available from: https://arxiv.org/abs/1712.09465 - 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
- Understanding close-lying exotic charmonia states within QCD sum rules
- Why 'ksi'(1690) and 'ksi'(2120) are so narrow?
- X(3872) production in high energy heavy ion collisions
- Understanding close-lying exotic charmonia states within QCD sum rules
- Update on J / 'psi' regeneration in a hadron gas
- On the absorption and production cross sections of 'K' and 'K' POT.*'
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