stephaneww
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The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
I don’t see why this matters. You can't compare G to another value, it's just a data in the equations, whereas you can compare energy densities by volume, and that's the problem with the vacuum catastrophe. You mean it's not important ? Thank you, I didn't know that. -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
Yes, but the vacuum catastrophe is dimensionless. No, it's Planck's energy (J: kg.m^2.t^-2) I made a mistake and corrected it later : (1)=mp.lp.tp2 is right (1) [math]\frac{m_p}{l_p.t_p^2}[/math] (J/m^3) is right I don't have another equation with F^2 I only have E^2=m^2c^4+p^2.c^2 to propose as a comparable example of a square. from a comparison of values in a spreadsheet where I have a whole series of physical values and relationships between them. Yes, but I also have no idea of the physical relevance of E^2. If you do, I'm interested -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
I suggest that QM is not of the same nature as relativity: I put the comological constant in a context of MQ by dimensional analysis. Here we find an extremely low energy density by volume The multiplication of the two square roots of the energy volume densities of the QM gives the value of the cosmological constant in relativity To my knowledge, there is no theory that includes square roots of energy volume density in QM, relativity or cosmology. (I know very little about QM and relativity) The only context in which I could find this dimension (J/m^3)^1/2 is with the Hildebrand solubility parameter I suggest that QM is not of the same nature as relativity: I put the comological constant in a context of MQ by dimensional analysis. Here we find an extremely low energy density by volume The multiplication of the two square roots of the energy volume densities of the QM gives the value of the cosmological constant in relativity To my knowledge, there is no theory that includes square roots of energy volume density in QM, relativity or cosmology. (I know very little about QM and relativity) The only context in which I could find this dimension (J/m^3)^1/2 is with the Hildebrand solubility parameter I don't know ooops error (1)=[math]\frac{m_p}{l_p.t^2}[/math] is right -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
and of course mission Planck is an experiment (shame on me ): https://en.wikipedia.org/wiki/Planck_(spacecraft) -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
I don't know if it's really from an experiment, but I use and datas from the Planck satellite from Wikipedia : [math] \Lambda=1,1056*10^{-52}.m^{-2}[/math] [math]\rho_{\Lambda}c^2=\frac{c^4 \Lambda}{8 \pi G}[/math] (2) and : [math]\frac{m_p.l_p^2}{t_p^2}[/math] (1) vaccum catastrophe = (1)/(2) Thank you, it was about Fp indeed. So a priori there's no physical sense of force squared... right ? In the same vein: does a squared pulse have a physical meaning in QM ? I ask the question because I've already seen it in an unpublished research work. Edit : The origin of the last messages after May comes from this thread: : https://www.scienceforums.net/topic/122287-puzzle-for-the-week-mystery-and-gum-ball-around-a-fine-structure-constant-in-planck-units-dimensioned-with-the-coulomb/ .. where I try to propose a link between the fine structure constant and the cosmological constant problem with this formula: : [math]\Large{\alpha=\frac {F_p^2}{e^2}. \frac {t_p^3}{m_p.2.\pi} . \frac {8.\pi^2}{c} .\frac {1}{\mu_0} }[/math] - [math]\alpha[/math]: fine constant structure - Fp: Planck's force - e : elementary charge - tp3/(mp.2.pi) : inverse of Planck's surface power density * 1/(2pi) note 1 : units of surface power density = W/m^2 = kg/s^3 note 2 : possible link with the problem of the cosmological constant ? - c : speed of light - μ0 : vacuum permeability -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
Yes, okay, but the pressure should decrease as the volume increases. But the pressure of the cosmological constant is constant as the volume increases. And I don't know what a square force is physically speaking to know if my "equality" can have a physical meaning -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
Yes, we've already talked about it, but for a force squared, what about it? -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
The simplicity of your argument had eluded me. Thank you. Edit : In the cosmological constant problem, there are no gravitational terms in the simplified formulas either, right ? -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
... The signs of the charges are opposite (electrically neutral universe), the Coulomb force is negative but its square is positive for example -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
yes, that help me, thank you 👍 after simplication the equality is correct and ... ...about of the doubt of the interest of the physical meaning of equality : I had note before that Fp = Coulomb's force with Planck's units ([math]q_1=q_2=q_p[/math] and [math]r=l_p[/math]) But I don't know if that equality can make physical sense with the problem of the cosmological constant with or whitout an electromagnetic framework . Do you have any idea ? About the Coulomb's force, there was a particular problem with the sign of the charges. . Can this "equality" help solve or am I going to fall back on circular reasoning... ? -
Okay, but not much of physical interest, except maybe something to do with the cosmological constant problem. [math]\Large{\frac {1}{\alpha}=\frac {F_p^2}{e^2}. \frac {t_p^3}{m_p.2.\pi} . \frac {8.\pi^2}{c} .\frac {1}{\mu_0} }[/math] - [math]\alpha[/math] : fine constant structure - [math]F_p[/math] : Planck's force - [math]e[/math] : elementary charge - [math] \Large{\frac {t_p^3}{m_p.2.\pi}} [/math] : inverse of Planck's surface power density * 1/(2pi) note 1 : units of surface power density = W/m^2 = kg/s^3 note 2 : possible link with the problem of the cosmological constant ? - [math]c[/math] : speed of light [math]\mu_0[/math] : vacuum permeability I would suggest the simplifications later in another message: too afraid to exceed the maximum editing time to correct the latex
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when you have a moment: enter in excel the exact values (from the formulas) of : - Planck's mass - Planck's length then the most accurate value [math]C [/math] of the Coulomb you can find. (6,24150962915265*10^18 elementary charge ) calculate the value of : [math]m_p.l_p/C^2*10^7[/math] estimate the numerical deviation in % from the inverse of the fine structure constant ([math]1/ \alpha[/math]) I find 0.00002%. Can you confirm please ? gauge the relevance in dimensional terms knowing that this calculation comes from this question: https://www.scienceforums.net/topic/118858-the-solution-of-the-cosmological-constant-problem/?do=findComment&comment=1118152 which also gives an acceptable approximation of the value of the vacuum catastrophe, but dimensioned, whereas the vacuum catastrophe is dimensionless. Please ___________________________________ basic working formula before simplification : [math](F_p^2/e^2)\text{ / Planck's surface density (in kg/s^3=W/^2)[]/math] - Fp: Planck force - e: elementary charge
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The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
ok -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
This proposal suits me. What title do you propose for the new thread ? -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
Me too Mordred 😉 -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
Hmm, no reaction, it's most probably a nonsense. -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
I confess I've lost track a little over the time... but is it foolish to consider the vacuum of the universe as a photon bath of the CMB as a support for an electromagnetic field that would fill the vacuum of the universe ? -
A connection between entropic gravity and the vacuum catastrophe ?
stephaneww replied to stephaneww's topic in Speculations
Hi Modred. About that : what do you think about this opinion please ? source : http://backreaction.blogspot.com/2019/09/the-five-most-promising-ways-to.html -
The solution of the Cosmological constant problem ?
stephaneww replied to stephaneww's topic in Speculations
ok (you omitted a c^2: [math]\rho_{\Lambda}=\frac{c^2 \Lambda}{8 \pi G_n}[/math] ) for the "quantum energy density of the vacuum" (B), if a temperature TB/m^3 = EB/kB/m^3 can be made to correspond, we have TB/m^3 = about 10^-110 K/m^3. There would be no absolute zero due again to the fluctuations of the quantum vacuum. (E=kB T) for the quantum mass density (A=10^96 kg/m^3) the mass of the current universe being 10^54 kg would be the index of a possible physical nonsense of this presentation, without it being a sufficient argument to prefer its value in K/m^3. as you suspect, the rest of your explanation escapes me, and in particular the reject of the use of the statistical mechanics of the mix edit : for the record, can you remind me what [math]U[/math] is, please?