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{\displaystyle -\omega } above, implying that a − ω {\displaystyle -\omega } relationship with the right-hand side of the quasi-geostrophic omega equation can…

de grupo son iguales: v=ωk=dωdk=c,{\displaystyle v={\frac {\omega }{k}}={\frac {d\omega }{dk}}=c,} donde c, es la velocidad de la luz en el vacío, que…

{\displaystyle \Omega _{\Lambda }} , la fracción de densidad de energía de un universo plano. En la actualidad, Ω Λ ≃ {\displaystyle \Omega _{\Lambda }\simeq…

pendulo parameter Real L=2; constant Real g=9.81; Real theta; Real omega; initial equation theta = 0.02; equation der(theta)=omega; der (omega)=-(g/L)*sin(theta);…

Kesler M.G., "A Generalized Thermodynamic Correlation Based on Three-Parameter Corresponding States", AIChE J., 21(3), 510-527, 1975 Reid R.C., Prausnitz…

experimental bounds on the contributions to the cosmological density parameter Ω{\displaystyle \Omega } from strongly interacting massive particles, ApJ 568, 1 (2002)…

\omega } , y parámetro α {\displaystyle \alpha } se vuelve f ( x ) = 2 ω ϕ ( x − ξ ω ) Φ ( α ( x − ξ ω ) ) . {\displaystyle f(x)={\frac {2}{\omega }}\phi…

Scientifiques, 66, 1988 (210-215). Bifurcations and Global Stability of Two-Parameter Families of Gradient Vector Fields with M. J. Carneiro, Publications Math…

probabilidad definido por ( Ω , F , P ) {\displaystyle (\Omega ,{\mathcal {F}},P)} , donde Ω {\displaystyle \Omega } es el espacio de muestra (esto es, el conjunto…

density contributed by dark energy, 0.76 ± 0.02, and the equation-of-state parameter, w ≈ −1 ± 0.1 (stat) ± 0.1 (sys), assuming that w is constant. This implies…

176ω2)(1−Tr0.5))2{\displaystyle \alpha =\left(1+\left(0.480+1.574\,\omega -0.176\,\omega ^{2}\right)\left(1-T_{r}^{\,0.5}\right)\right)^{2}}, a=19(23−1)R2Tc2Pc=0…

2008: 1-10. doi:10.1155/2008/685175.  Shi, Y.; Eberhart, R.C. (1998). «Parameter selection in particle swarm optimization». Proceedings of Evolutionary…

\left(\omega _{mn}t\right)} donde m,n son enteros no nulos, Amn son constantes arbitrarias y ωmn2=c2(m2π2L12+n2π2L22).{\displaystyle \omega _{mn}^{2}=c^{2}\left({\frac…

Omega }_{\alpha 1}}&{{\Omega }_{\alpha 2}}&{{\Omega }_{\alpha 3}}\\{{\Omega }_{\beta 1}}&{{\Omega }_{\beta 2}}&{{\Omega }_{\beta 3}}\\{{\Omega }_{\gamma…

speed number Weissenberg number Womersley number «Lockhart–Martinelli parameter». Archivado desde el original el 15 de noviembre de 2009. Consultado el…

1016/s0167-5060(08)70044-x .. Knauer, Christian; Spillner, Andreas (2006), «A fixed-parameter algorithm for the minimum weight triangulation problem based on small…

1925;19(2):338-9. PMID 16743508 Tseng SJ, Hsu JP. A comparison of the parameter estimating procedures for the Michaelis–Menten model. J Theor Biol. 1990…

1103/PhysRevD.59.067702.  Johannes Hirn and Verónica Sanz (2006). «Negative S Parameter from Holographic Technicolor». Physical Review Letters 97 (12): 121803…

WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS». The Astrophysical Journal Supplement Series 208 (2): 19. ISSN 0067-0049…