Source: PHYSICAL REVIEW D. Unidade: IAG
Subjects: MATÉRIA ESCURA, ENERGIA, SUPERNOVAS, RAIOS GAMA
ABNT
BUSTI, V. C e SANTOS, R. C e LIMA, Jose Ademir Sales de. Constraining the dark energy and smoothness parameter with type Ia supernovae and gamma-ray bursts. PHYSICAL REVIEW D, v. 85, p. 103503/1-103503/8, 2012Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.85.103503. Acesso em: 10 nov. 2024.APA
Busti, V. C., Santos, R. C., & Lima, J. A. S. de. (2012). Constraining the dark energy and smoothness parameter with type Ia supernovae and gamma-ray bursts. PHYSICAL REVIEW D, 85, 103503/1-103503/8. doi:10.1103/PhysRevD.85.103503NLM
Busti VC, Santos RC, Lima JAS de. Constraining the dark energy and smoothness parameter with type Ia supernovae and gamma-ray bursts [Internet]. PHYSICAL REVIEW D. 2012 ; 85 103503/1-103503/8.[citado 2024 nov. 10 ] Available from: https://doi.org/10.1103/PhysRevD.85.103503Vancouver
Busti VC, Santos RC, Lima JAS de. Constraining the dark energy and smoothness parameter with type Ia supernovae and gamma-ray bursts [Internet]. PHYSICAL REVIEW D. 2012 ; 85 103503/1-103503/8.[citado 2024 nov. 10 ] Available from: https://doi.org/10.1103/PhysRevD.85.103503