Arterial pulsation-driven cerebrospinal fluid flow in the perivascular space: a computational model.
This study was conducted to determine whether local arterial pulsations are sufficient to cause cerebrospinal fluid (CSF) flow along perivascular spaces (PVS) within the spinal cord. A theoretical model of the perivascular space surrounding a "typical" small artery was analysed using computational fluid dynamics. Systolic pulsations were modelled as travelling waves on the arterial wall. The effects of wave geometry and variable pressure conditions on fluid flow were investigated. Arterial pulsations induce fluid movement in the PVS in the direction of arterial wave travel. Perivascular flow continues even in the presence of adverse pressure gradients of a few kilopascals. Flow rates are greater with increasing pulse wave velocities and arterial deformation, as both an absolute amplitude and as a proportion of the PVS. The model suggests that arterial pulsations are sufficient to cause fluid flow in the perivascular space even against modest adverse pressure gradients. Local increases in flow in this perivascular pumping mechanism or reduction in outflow may be important in the etiology of syringomyelia.
Bilston
Lynne E
LE
Prince of Whales Medical Research Institute, University of New South Whales, Barker St, Randwick, NSW 2031, Australia. l.bilston@unsw.edu.au
Fletcher
David F
DF
Brodbelt
Andrew R
AR
Stoodley
Marcus A
MA
D001158:Arteries / Q000502:physiology*; D001794:Blood Pressure / Q000502:physiology; D015170:Cerebrospinal Fluid Pressure / Q000502:physiology*; D003198:Computer Simulation; D008955:Models, Cardiovascular; D011673:Pulsatile Flow / Q000502:physiology*; D013116:Spinal Cord / Q000098:blood supply* / Q000502:physiology*