Note, that micro black holes last within micro seconds, and that we wish to ascertain how to build, in a laboratory, a black hole, which may exist say at least up to 10^?1 seconds and provide a test bed as to early un...Note, that micro black holes last within micro seconds, and that we wish to ascertain how to build, in a laboratory, a black hole, which may exist say at least up to 10^?1 seconds and provide a test bed as to early universe gravitational theories. First of all, it would be to determine, if the mini black hole bomb, would spontaneously occur, unless the Kerr-Newmann black hole were carefully engineered in the laboratory. Specifically, we state that this paper is modeling the creation of an actual Kerr Newman black hole via laser physics, or possibly by other means. We initiate a model of an induced Kerr-Newman black Holes, with specific angular momentum J, and then from there model was to what would happen as to an effective charge, Q, creating an E and B field, commensurate with the release of GWs. The idea is that using a frame of reference trick, plus E + i B = ?function of the derivative of a complex valued scalar field, as given by Appell, in 1887, and reviewed by Whittaker and Watson, 1927 of their “A Course of Modern Analysis” tome that a first principle identification of a B field, commensurate with increase of thermal temperature, T, so as to have artificially induced GW production. This is compared in part with the Park 1955 paper of a spinning rod, producing GW, with the proviso that both the spinning rod paper, and this artificial Kerr-Newman Black hole will employ the idea of lasers in implementation of their respective GW radiation. The idea is in part partly similar to an idea the author discussed with Dr. Robert Baker, in 2016 with the difference that a B field would be generated and linked to effects linked with induced spin to the Kerr-Newman Black hole. We close with some observations about the “black holes have no hair” theorem, and our problem. Citing some recent suppositions that this “theorem” may not be completely true and how that may relate to our experimental situation. We close with observations from Haijicek, 2008 as which may be pertinent to Quantization of Gravity. Furthermore as an answer to questions raised by a referee, we will have a final statement as to how this problem is for a real black hole being induced, and answering his questions in his review, which will be included in a final appendix to this paper. The main issue which is now to avoid the black hole bomb effect which would entail an explosion of a small black hole in a laboratory. Furthermore as an answer to questions raised by a referee, we will have a final statement as to how this problem is for a real black hole being induced, and answering his questions in his review, which will be included in a final appendix to this paper. In all, the main end result is to try to avoid the so called black hole bomb effect, where a mini black hole would explode in a laboratory setting within say 10^?16 or so seconds, i.e. the idea would be to have a reasonably stable configuration within put laser energy, but a small mass, and to do it over hopefully 10^15 or more times longer than the 10^?16 seconds where the mini black hole would quickly evaporate. I.e. a duration of say up to 10^?1 seconds which would provide a base line as to astrophysical modeling of a Kerr-Newman black hole.展开更多
We claim that the linking of a shrinking prior universe to our own via a wormhole bridge solution of about ten to the minus forty four power seconds permits the formation of a short-term quintessence scalar field. Sym...We claim that the linking of a shrinking prior universe to our own via a wormhole bridge solution of about ten to the minus forty four power seconds permits the formation of a short-term quintessence scalar field. Symmetries allow for creating high-frequency gravitational waves at the onset of inflation, which has consequences in our present cosmological era. This instantaneous energy transfer between prior to present universes permits relic graviton production which we claim is a viable candidate for future propulsion technologies in space craft design. The Big Bang started as the passage of thermal energy from an existing universe into ours resulting in another Big Bang, and helps us understand how a graviton burst can occur in the first place.展开更多
In a prior paper, the d = 1 to d = 7 sense of AdS/CFT solutions were described in general whereas we did not introduce commentary as to GW polarization of gravitational radiation from a worm hole. We will discuss GW p...In a prior paper, the d = 1 to d = 7 sense of AdS/CFT solutions were described in general whereas we did not introduce commentary as to GW polarization of gravitational radiation from a worm hole. We will discuss GW polarization, for d = 1 and in addition say concrete facts as to the strength of the GW radiation, and admissible frequencies. First off, the term Δt is for the smallest unit of time step. Note that in the small Δt limit for d = 1 we avoid any imaginary time no matter what the sign of Ttemp is. And when d = 1 in order to have any solvability one would need X = Δt assumed to be infinitesimal. To first approximation, we set X = Δt as being of Planck time, 10-31 or so seconds, in duration.展开更多
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 m...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.展开更多
Note, in a prior paper, we ascertained physics thought experiment configuration for a black hole, which may exist say at least up to 10-1 seconds. Our idea was to experimentally provide a test bed as to early universe...Note, in a prior paper, we ascertained physics thought experiment configuration for a black hole, which may exist say at least up to 10-1 seconds. Our idea was to experimentally provide a test bed as to early universe gravitational theories. In doing so, we as follow up to that black hole paper come up with a criteria as to Quintic polynomial with regards to Δt which is the interval of time for which we can measure (down to Planck time) the production of Gravitational waves and gravitons, from an induced Kerr-Newman black hole. In doing so we access what is given in an AdS/CFT rendition of black hole entropy written by Pires which gives an input strategy as to how to relate Δt to a (Δt)5 + A1 ? (Δt)2 + A2 =0 Quintic polynomial which has only a few combinations which may be exactly solvable. We find that A2 has a number, n of presumed produced gravitons, in the time interval Δt and that both A1 and A2 have an Ergosphere area, due to the induced Kerr-Newman black hole. Finally, we extract information via the use of the Uncertainty Principle, as to ΔEΔt ≥ ? with ΔE ∝ E0 ≡ mc2, so if we have a mass m, we will be able to extract Δt. This due to very complete arguments as to Kerr-Newman black holes, which when we have entropy, due to the Infinite quantum statistics argument given by Ng, leads to a counting algorithm, of n gravitons, which is proportional to entropy during which is then leading directly to fixing Δt directly via us of (Δt)5 + A1 ? (Δt)2 + A2 =0, with the Quintic evaluated according to Blair K. Spearman and Kenneth S. Williams, in the Rocky mountain journal of mathematics, as of 1996. i.e. if this polynomial, as by our described Quintic polynomial, in Δt, (Δt)5 + A1 ? (Δt)2 + A2 =0 is exactly solvable, then our Kerr Newman black hole is leading to quantum gravity. Otherwise, gravity in its foundations with respect to the Kerr Newman blackhole is classical to semi classical. In its characterization of gravity. Note that specifically, we state that this paper is modeling the creation of an actual Kerr Newman black hole via laser physics, or possibly by other means and that our determination of Δt as being solved, exactly by (Δt)5 + A1 ? (Δt)2 + A2 =0 is our way of determining if the Kerr Newman black hole leads to quantum gravity.展开更多
To some extent,the operational quickness of semiconductor devices depends on the transmission time of an electron through semiconductor nanostructures.However,the calculation of transmission time is very difficult,tha...To some extent,the operational quickness of semiconductor devices depends on the transmission time of an electron through semiconductor nanostructures.However,the calculation of transmission time is very difficult,thanks to both the contentious definition of the transmission time in quantum mechanics and the complicated effective potential functions experienced by electrons in semiconductor devices.Here,based on an improved transfer matrix method to numerically solve the Schr?dinger equation and H G Winful’s relationship to calculate the dwell time,we develop a numerical approach to evaluate the transmission time of an electron in semiconductor devices.Compared to the exactly resolvable case of the rectangular potential barrier,the established numerical approach possesses high precision and small error,which may be employed to explore the dynamic response and operating speed of semiconductor devices.This proposed numerical method is successfully applied to the calculation of dwell time for an electron in double rectangular potential barriers and the dependence of transmission time on the number of potential barriers is revealed.展开更多
文摘Note, that micro black holes last within micro seconds, and that we wish to ascertain how to build, in a laboratory, a black hole, which may exist say at least up to 10^?1 seconds and provide a test bed as to early universe gravitational theories. First of all, it would be to determine, if the mini black hole bomb, would spontaneously occur, unless the Kerr-Newmann black hole were carefully engineered in the laboratory. Specifically, we state that this paper is modeling the creation of an actual Kerr Newman black hole via laser physics, or possibly by other means. We initiate a model of an induced Kerr-Newman black Holes, with specific angular momentum J, and then from there model was to what would happen as to an effective charge, Q, creating an E and B field, commensurate with the release of GWs. The idea is that using a frame of reference trick, plus E + i B = ?function of the derivative of a complex valued scalar field, as given by Appell, in 1887, and reviewed by Whittaker and Watson, 1927 of their “A Course of Modern Analysis” tome that a first principle identification of a B field, commensurate with increase of thermal temperature, T, so as to have artificially induced GW production. This is compared in part with the Park 1955 paper of a spinning rod, producing GW, with the proviso that both the spinning rod paper, and this artificial Kerr-Newman Black hole will employ the idea of lasers in implementation of their respective GW radiation. The idea is in part partly similar to an idea the author discussed with Dr. Robert Baker, in 2016 with the difference that a B field would be generated and linked to effects linked with induced spin to the Kerr-Newman Black hole. We close with some observations about the “black holes have no hair” theorem, and our problem. Citing some recent suppositions that this “theorem” may not be completely true and how that may relate to our experimental situation. We close with observations from Haijicek, 2008 as which may be pertinent to Quantization of Gravity. Furthermore as an answer to questions raised by a referee, we will have a final statement as to how this problem is for a real black hole being induced, and answering his questions in his review, which will be included in a final appendix to this paper. The main issue which is now to avoid the black hole bomb effect which would entail an explosion of a small black hole in a laboratory. Furthermore as an answer to questions raised by a referee, we will have a final statement as to how this problem is for a real black hole being induced, and answering his questions in his review, which will be included in a final appendix to this paper. In all, the main end result is to try to avoid the so called black hole bomb effect, where a mini black hole would explode in a laboratory setting within say 10^?16 or so seconds, i.e. the idea would be to have a reasonably stable configuration within put laser energy, but a small mass, and to do it over hopefully 10^15 or more times longer than the 10^?16 seconds where the mini black hole would quickly evaporate. I.e. a duration of say up to 10^?1 seconds which would provide a base line as to astrophysical modeling of a Kerr-Newman black hole.
文摘We claim that the linking of a shrinking prior universe to our own via a wormhole bridge solution of about ten to the minus forty four power seconds permits the formation of a short-term quintessence scalar field. Symmetries allow for creating high-frequency gravitational waves at the onset of inflation, which has consequences in our present cosmological era. This instantaneous energy transfer between prior to present universes permits relic graviton production which we claim is a viable candidate for future propulsion technologies in space craft design. The Big Bang started as the passage of thermal energy from an existing universe into ours resulting in another Big Bang, and helps us understand how a graviton burst can occur in the first place.
文摘In a prior paper, the d = 1 to d = 7 sense of AdS/CFT solutions were described in general whereas we did not introduce commentary as to GW polarization of gravitational radiation from a worm hole. We will discuss GW polarization, for d = 1 and in addition say concrete facts as to the strength of the GW radiation, and admissible frequencies. First off, the term Δt is for the smallest unit of time step. Note that in the small Δt limit for d = 1 we avoid any imaginary time no matter what the sign of Ttemp is. And when d = 1 in order to have any solvability one would need X = Δt assumed to be infinitesimal. To first approximation, we set X = Δt as being of Planck time, 10-31 or so seconds, in duration.
基金This work is supported in part by National Nature Science Foundation of China grant No.11375279.
文摘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.
文摘Note, in a prior paper, we ascertained physics thought experiment configuration for a black hole, which may exist say at least up to 10-1 seconds. Our idea was to experimentally provide a test bed as to early universe gravitational theories. In doing so, we as follow up to that black hole paper come up with a criteria as to Quintic polynomial with regards to Δt which is the interval of time for which we can measure (down to Planck time) the production of Gravitational waves and gravitons, from an induced Kerr-Newman black hole. In doing so we access what is given in an AdS/CFT rendition of black hole entropy written by Pires which gives an input strategy as to how to relate Δt to a (Δt)5 + A1 ? (Δt)2 + A2 =0 Quintic polynomial which has only a few combinations which may be exactly solvable. We find that A2 has a number, n of presumed produced gravitons, in the time interval Δt and that both A1 and A2 have an Ergosphere area, due to the induced Kerr-Newman black hole. Finally, we extract information via the use of the Uncertainty Principle, as to ΔEΔt ≥ ? with ΔE ∝ E0 ≡ mc2, so if we have a mass m, we will be able to extract Δt. This due to very complete arguments as to Kerr-Newman black holes, which when we have entropy, due to the Infinite quantum statistics argument given by Ng, leads to a counting algorithm, of n gravitons, which is proportional to entropy during which is then leading directly to fixing Δt directly via us of (Δt)5 + A1 ? (Δt)2 + A2 =0, with the Quintic evaluated according to Blair K. Spearman and Kenneth S. Williams, in the Rocky mountain journal of mathematics, as of 1996. i.e. if this polynomial, as by our described Quintic polynomial, in Δt, (Δt)5 + A1 ? (Δt)2 + A2 =0 is exactly solvable, then our Kerr Newman black hole is leading to quantum gravity. Otherwise, gravity in its foundations with respect to the Kerr Newman blackhole is classical to semi classical. In its characterization of gravity. Note that specifically, we state that this paper is modeling the creation of an actual Kerr Newman black hole via laser physics, or possibly by other means and that our determination of Δt as being solved, exactly by (Δt)5 + A1 ? (Δt)2 + A2 =0 is our way of determining if the Kerr Newman black hole leads to quantum gravity.
基金supported jointly by the National Natural Science Foundation of China(11864009 and 62164005)the Guangxi Natural Science Foundation of China(2021JJB110053)
文摘To some extent,the operational quickness of semiconductor devices depends on the transmission time of an electron through semiconductor nanostructures.However,the calculation of transmission time is very difficult,thanks to both the contentious definition of the transmission time in quantum mechanics and the complicated effective potential functions experienced by electrons in semiconductor devices.Here,based on an improved transfer matrix method to numerically solve the Schr?dinger equation and H G Winful’s relationship to calculate the dwell time,we develop a numerical approach to evaluate the transmission time of an electron in semiconductor devices.Compared to the exactly resolvable case of the rectangular potential barrier,the established numerical approach possesses high precision and small error,which may be employed to explore the dynamic response and operating speed of semiconductor devices.This proposed numerical method is successfully applied to the calculation of dwell time for an electron in double rectangular potential barriers and the dependence of transmission time on the number of potential barriers is revealed.
