He has just started with the simplest of all the Schwarzchild Metric, that probably confused you to call it a river metric...
.............In the river model, space itself flows like a river through a flat background.....This is what he says, now please tell me which 'metric' would have a flat background ? And what is that flat background ?
Why are you arguing ? Its a model for lay people to get some ideas about BH. Please don't call it a metric, which is a precise representation of 4-D spacetime geometry...
Oh Brother!!!
http://arxiv.org/pdf/gr-qc/0411060.pdf
Abstract:
This paper presents an under-appreciated way to conceptualize stationary black holes, which we call the river model. The river model is mathematically sound, yet simple enough that the basic picture can be understood by non-experts. In the river model, space itself flows like a river through a flat background, while objects move through the river according to the rules of special relativity. In a spherical black hole, the river of space falls into the black hole at the Newtonian escape velocity, hitting the speed of light at the horizon. Inside the horizon, the river flows inward faster than light, carrying everything with it. We show that the river model works also for rotating (Kerr-Newman) black holes, though with a surprising twist. As in the spherical case, the river of space can be regarded as moving through a flat background. However, the river does not spiral inward, as one might have anticipated, but rather falls inward with no azimuthal swirl at all. Instead, the river has at each point not only a velocity but also a rotation, or twist. That is, the river has a Lorentz structure, characterized by six numbers (velocity and rotation), not just three (velocity). As an object moves through the river, it changes its velocity and rotation in response to tidal changes in the velocity and twist of the river along its path. An explicit expression is given for the river field, a six-component bivector field that encodes the velocity and twist of the river at each point, and that encapsulates all the properties of a stationary rotating black hole.
""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""
In summing, Professor Hamilton and his colleagues on his wb site also confirms that due to the more complicated nature of Reisnner-Nordstrom solution metric, he is working at this time is applying it to all BH's generally.
True as we all know since the simple Schwarzchild metric was formulated during the WW1, while Roy Kerr did not have a solution to the type that bears his name until 1963.
Yet this model is also applicable to Kerr type.
Perhaps you my friend [you meaning the god] would like to submit another paper correcting Professor Hamilton's paper.
I won't hold my breath though.