Changes

Quantised Inertia combines these two predictions by saying that the horizon damps the Unruh waves on one side of the object—rather as sea defences damp ocean waves. The resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.<ref> {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}</ref><ref> {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}</ref>

Quantised Inertia combines these two predictions by saying that the horizon damps the Unruh waves on one side of the object—rather as sea defences damp ocean waves. The resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.<ref> {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}</ref><ref> {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}</ref>

Furthermore, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon. As such, the waves of Unruh radiation are now damped equally all around, and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.<ref> {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics & Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}</ref><ref> {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics & Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}</ref>

Quantised Inertia further predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon. As such, the waves of Unruh radiation are now damped equally all around, and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.<ref> {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics & Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}</ref><ref> {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics & Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}</ref>

==References==

==References==