## LIGO blackhole anomaly and minimal surface model for star
The TGD inspired model of star as a minimal surface with stationary spherically symmetric metric suggests strongly that the analog of blackhole metric as two horizons. The outer horizon is analogous to Scwartschild horizon in the sense that the roles of time coordinate and radial coordinate change. Radial metric component vanishes at Scwartschild horizon rather than divergence. Below the inner horizon the metric has Eucldian signature.
Is there any empirical evidence for the existence of two horizons? There is evidence that the formation of the recently found LIGO blackhole (discussed from TGD view point in is not fully consistent with the GRT based model (see this). There are some indications that LIGO blackhole has a boundary layer such that the gravitational radiation is reflected forth and back between the inner and outer boundaries of the layer. In the proposed model the upper boundary would not be totally reflecting so that gravitational radiation leaks out and gave rise to echoes at times .1 sec, .2 sec, and .3 sec. It is perhaps worth of noticied that time scale .1 sec corresponds to the secondary p-adic time scale of electron (characterized by Mersenne prime M
The proposed model (see this) assumes that the inner horizon is Schwarstchild horizon. TGD would however suggests that the outer horizon is the TGD counterpart of Schwartschild horizon. It could have different radius since it would not be a singularity of g
One should understand why it takes rather long time T=.1 seconds for radiation to travel forth and back the distance L= r
Δ m
Δ t = ∫ The time needed to travel forth and back does not depend on h and would be given by
Δ m
This time cannot be shorter than the minimal time (r
There is an intriguing connection with the notion of gravitational Planck constant. The formula for gravitational Planck constant given by h See the new chapter Can one apply Occam's razor as a general purpose debunking argument to TGD? or article with the same title. |