摘要
First off,the termΔt is for the smallest unit of time step.Now,due to reasons we will discuss we state that,contrary to the wishes of a reviewer,the author asserts that a full Galois theory analysis of a quintic is mandatory for reasons which reflect about how the physics answers are all radically different for abbreviated lower math tech answers to this problem.i.e.if one turns the quantic to a quadratic,one gets answers materially different from when one applies the Gauss-Lucas theorem.So,despite the distaste of some in the physics community,this article pitches Galois theory for a restricted quintic.We begin our analysis of if a quintic equation for a shift in time,as for a Kerr Newman black hole affects possible temperature values,which may lead to opening or closing of a worm hole throat.Following Juan Maldacena,et al.,we evaluate the total energy of a worm hole,with the proviso that the energy of the worm hole,in four dimensions for a closed throat has energy of the worm hole,as proportional to negative value of(temperature times a fermionic number,q)which is if we view a worm hole as a connection between two black holes,a way to show if there is a connection between quantization of gravity,and if the worm hole throat is closed.Or open.For the quantic polynomial,we relateΔt to a(Δt)^(5)+A_(1)·(Δt)^(2)+A_(2)=0 Quintic polynomial which has several combinations which Galois theoretical sense is generally solvable.We find that A_(2)has a number,n of presumed produced gravitons,in the time intervalΔt and that both A_(1)and A_(2)have an Ergosphere area,due to the induced Kerr-Newman black hole.If Gravitons and Gravitinos have the relationship the author purports in an article the author wrote years ago,as cited in this publication,then we have a way to discuss if quantization of gravity as affecting temperature T,in the worm hole tells us if a worm hole is open or closed.And a choice of the solvable constraints affects temperature,T,which in turn affects the sign of a worm hole throat is far harder to solve.We explain the genesis of black hole physics negative temperature which is necessary for a positive black hole entropy,and then state our results have something very equivalent in terms of worm ding(Δt)^(5)+A_(1)·(Δt)^(2)+A_(2)=0 we will be having X=Δt assumed to be negligible,We then look at a quadratic version in the solution of X=Δt so we are looking at four regimes for solving a quintic,with the infinitesimal value ofΔt effectively reduced our quintic to a quadratic equation.Note that in the smallΔt limit for d=1,3,5,7,we cleanly avoid any imaginary time no matter what the sign of T_(temp)is.In the case where we have X=Δt assumed to be negligible,the connection in our text about coupling constants,if d=3,may in itself for infinitesimalΔt lend toward supporting d=3.This is different from the more general case for general Galois solvability of(Δt)^(5)+A_(1)·(Δt)^(2)+A_(2)=0.d≠1 means we need to consider Galois theory.If d=2,4,6,need T_(temp)A_(1)to be greater than zero.If d≠1 and is instead d=3,5,7,there is an absence of general solutions in the Galois solution sense.This because if.d≠1 A_(1)<0 whenever d=3,5,7.And when d=1 in order to have any solvability one would need X=Δt assumed to be infinitesimal in(Δt)^(5)+A_(1)·(Δt)^(2)+A_(2)=0.
基金
This work is supported in part by National Nature Science Foundation of China grant No.11375279.
