The Bagnold number (Ba) is the ratio of grain collision stresses to viscous fluid stresses in a granular flow with interstitial Newtonian fluid, first identified by Ralph Alger Bagnold.[1]
The Bagnold number is defined by
-
B
a
=
ρ
d
2
λ
1
/
2
γ
˙
μ
{\displaystyle \mathrm {Ba} ={\frac {\rho d^{2}\lambda ^{1/2}{\dot {\gamma }}}{\mu }}}
,[2]
where
ρ
{\displaystyle \rho }
is the particle density,
d
{\displaystyle d}
is the grain diameter,
γ
˙
{\displaystyle {\dot {\gamma }}}
is the shear rate and
μ
{\displaystyle \mu }
is the dynamic viscosity of the interstitial fluid. The parameter
λ
{\displaystyle \lambda }
is known as the linear concentration, and is given by
-
λ
=
1
(
ϕ
0
/
ϕ
)
1
3
−
1
{\displaystyle \lambda ={\frac {1}{\left(\phi _{0}/\phi \right)^{\frac {1}{3}}-1}}}
,
where
ϕ
{\displaystyle \phi }
is the solids fraction and
ϕ
0
{\displaystyle \phi _{0}}
is the maximum possible concentration (see random close packing).
In flows with small Bagnold numbers (Ba < 40), viscous fluid stresses dominate grain collision stresses, and the flow is said to be in the "macro-viscous" regime. Grain collision stresses dominate at large Bagnold number (Ba > 450), which is known as the "grain-inertia" regime. A transitional regime falls between these two values.
See also
References
- Bagnold, R. A. (1954). "Experiments on a Gravity-Free Dispersion of Large Solid Spheres in a Newtonian Fluid under Shear". Proc. R. Soc. Lond. A. 225 (1160): 49–63. Bibcode:1954RSPSA.225...49B. doi:10.1098/rspa.1954.0186. S2CID 98030586.
- Hunt, M. L.; Zenit, R.; Campbell, C. S.; Brennen, C.E. (2002). "Revisiting the 1954 suspension experiments of R. A. Bagnold". Journal of Fluid Mechanics. 452 (1): 1–24. Bibcode:2002JFM...452....1H. CiteSeerX 10.1.1.564.7792. doi:10.1017/S0022112001006577. S2CID 9416685.
External links