We describe the haemodynamics in the individual capillaries using Poiseuille’s equation [29 (link)], where the volumetric flow rate in a vessel is related to the pressure drop across it via
where μB the blood viscosity, R is the capillary lumen radius with cross-sectional area πR2, and Lvsc is the length of a capillary segment. Note that R and Lvsc change in time since vessels are deformed under solid stresses. The blood viscosity is assumed homogeneous and constant in time; this is in order to remove an additional model parameter in lieu of suitable data with which to inform it. Interstitial fluid flow is described using Darcy’s law [33 (link), 34 (link)] so that the volumetric fluid flow rate in the extracellular space is given by
where Kint is the hydraulic conductivity of the interstitium, Aint is the interstitium cross-sectional area, and Lint is the length of a tissue segment whose interstitial fluid pressure difference is denoted by Δpint. The cross-sectional area can be expressed with respect to the mean capillary radius and the vascular density, Svsc, as [35 (link)]. Here is the average capillary radius in the local neighbourhood of the connective tissues under consideration.
To model the fluid movement across the capillary barrier that occurs as a result of filtration, we use Starling’s equation. Similarly to Baish at al. [35 (link)], the volumetric transvascular flow rate across the permeable endothelium is expressed through Starling’s law
Here Kvsc is the hydraulic conductivity of the endothelial barrier, which can be expressed as a function of the size of the fenestrations on the vessel (pores’ average radius), rp, the fraction of vessel-wall surface occupied by pores, γp, and the blood viscosity, μB, via [36 (link)]:
Finally, Avsc is the surface area of the blood vessel wall and the “effective” pressure is given by
where σo is the average osmotic reflection coefficient of the plasma proteins, πvsc is the osmotic pressure of the plasma at the permeable vascular wall, while πint is the corresponding osmotic pressure of the interstitial fluid. This modelling approach accounts for the contribution of the colloid osmotic pressure of plasma and interstitial fluid. Including those features are important for a complete modelling description of the micro-circulation system. Nonetheless, numerical experiments have revealed that the omission of the rightmost term inEq (8) in the vascular–interstitium interaction model has only marginally affected the qualitative predictions of the proposed tumour-growth angiogenesis model. This is also supported by the experimental findings of Tong and colleagues [37 (link)], who showed that the osmotic pressure difference across the wall of tumour vessels is negligible.
It is important to note here that we do not include the lymphatic system in the current model, given that it is generally assumed to be compromised in tumour tissues. However, this would be a straightforward extension to the current framework.
The flow rate Eqs (4 )–(6 ) are coupled to a model for the vascular and interstitial pressures. In the vascular network, conservation of fluid flux at vessel junctions provides a linear system of equations to solve for the nodal pressures, subject to pressure/flow boundary conditions on the terminal nodal points of the network. The interstitial pressure, pint, satisfies the Poisson equation, where the source term captures both vascular and osmotic contributions, following the approach of Stylianopoulos and Jain [26 (link)]. Quasi-steady state fluid flow is solved numerically for the vascular and interstitial pressures (defined on nodal points in the vascular network, and extravascular-space points, respectively). An interconnected grid of tissue and vascular nodes is considered. Tissue nodes are connected to each other via the 3D FE mesh, where each tissue element corresponds to a two node edge element of the FE grid. Vascular nodes are connected to each other according to the network structure generated by the vascular network module, defined in the Angiogenesis model subsection. Also, as shown in the 2D illustration of Fig 1C , each vascular node is contained in a FE of the discrete three-dimensional domain of analysis. Thus, in order to describe transvascular flow through Eq (6) , each vascular node is associated with the corresponding vertices (i.e. tissue nodes) of the FE.
After every simulation of the flow model, the magnitude of the average wall shear stress (WSS) distribution, τf, the axial blood-flow mean velocity in a vascular segment, vvsc, and the fluid velocity at the interstitium, vint, can be evaluated using the following relationships:
where Δpvsc and Δpint is the pressure difference between two vascular and two interstitial nodes respectively of the corresponding discretised domains of analysis (i.e. the vascular network and the ECM) respectively. The value set for the material parameters of the above equations are provided separately inS2 Table .
where μB the blood viscosity, R is the capillary lumen radius with cross-sectional area πR2, and Lvsc is the length of a capillary segment. Note that R and Lvsc change in time since vessels are deformed under solid stresses. The blood viscosity is assumed homogeneous and constant in time; this is in order to remove an additional model parameter in lieu of suitable data with which to inform it. Interstitial fluid flow is described using Darcy’s law [33 (link), 34 (link)] so that the volumetric fluid flow rate in the extracellular space is given by
where Kint is the hydraulic conductivity of the interstitium, Aint is the interstitium cross-sectional area, and Lint is the length of a tissue segment whose interstitial fluid pressure difference is denoted by Δpint. The cross-sectional area can be expressed with respect to the mean capillary radius and the vascular density, Svsc, as [35 (link)]. Here is the average capillary radius in the local neighbourhood of the connective tissues under consideration.
To model the fluid movement across the capillary barrier that occurs as a result of filtration, we use Starling’s equation. Similarly to Baish at al. [35 (link)], the volumetric transvascular flow rate across the permeable endothelium is expressed through Starling’s law
Here Kvsc is the hydraulic conductivity of the endothelial barrier, which can be expressed as a function of the size of the fenestrations on the vessel (pores’ average radius), rp, the fraction of vessel-wall surface occupied by pores, γp, and the blood viscosity, μB, via [36 (link)]:
Finally, Avsc is the surface area of the blood vessel wall and the “effective” pressure is given by
where σo is the average osmotic reflection coefficient of the plasma proteins, πvsc is the osmotic pressure of the plasma at the permeable vascular wall, while πint is the corresponding osmotic pressure of the interstitial fluid. This modelling approach accounts for the contribution of the colloid osmotic pressure of plasma and interstitial fluid. Including those features are important for a complete modelling description of the micro-circulation system. Nonetheless, numerical experiments have revealed that the omission of the rightmost term in
It is important to note here that we do not include the lymphatic system in the current model, given that it is generally assumed to be compromised in tumour tissues. However, this would be a straightforward extension to the current framework.
The flow rate Eqs (
After every simulation of the flow model, the magnitude of the average wall shear stress (WSS) distribution, τf, the axial blood-flow mean velocity in a vascular segment, vvsc, and the fluid velocity at the interstitium, vint, can be evaluated using the following relationships:
where Δpvsc and Δpint is the pressure difference between two vascular and two interstitial nodes respectively of the corresponding discretised domains of analysis (i.e. the vascular network and the ECM) respectively. The value set for the material parameters of the above equations are provided separately in