Jump to content

conservation of the energy of the universe ???

Featured Replies

Hi,

I have in the idea that the decrease of the temperature of the universe and the expansion of the universe are compensated exactly in terms of energies and propose the following calculations

age of the universe (recombination) 378 000 years, with temperature CMB T1 = 3000 K, redshift  : z1= 1 100, radius observable universe : R1 = 3.96*10^23 m

age of the universe today : 13.797.000.000 years, with temperature CMB T0 = 2.725 K, reshift  z0=1, radius observable universe R0 = 4.36*10^26 m and [latex]H_0=67.74[/latex], 

z1=T1/T0

z1=3000K/2.725K=1100

R0 = (1+z) * R1 ,

V1 = 2.59 * 10^71 m^3,

V0 = 3.47 * 10^80 m^3.

(Vt = volume of observable universe )

[latex]H_{t1}=H_0*\sqrt{\Omega_m(1+z)^3+\Omega_{\text{rad}}(1+z)^4+\Omega_{\Lambda} }=158284\text{ km/s/Mpc}[/latex]

with :

[latex]\Omega_m=0.3089[/latex]

[latex]\Omega_{\text{rad}}=9*10^{-5}[/latex]

[latex]\Omega_{\Lambda}=0.6911[/latex]

__________________________________________________________

[latex]V_t [/latex] : Volume of observable universe

Boltzmann constant : [latex]k_B = 1.380 648 52 * 10^{-23}J/K[/latex]

[latex]X1=k_B*T_1/V_1=1.38*10^{-23}*3000/(2.59*10^{71})=1.60*10^{-91}J/m^3[/latex]

[latex]X0=k_B*T_0/V_0=1.38*10^{23}*2.725/(3.47*10^{80})=1.09*10^{-103}J/m^3[/latex]

[latex](X1/X0)/(\Omega_m(1+z)^3+\Omega_{\text{rad}}(1+z)^4+\Omega_{\Lambda})=(1.47*10^{12})/(5.46*10^8)=2697[/latex] dimensionless

[latex]M_t[/latex] : "total mass" of observable universe  (for its energy do [latex]M_t* c^2[/latex], the next ratio is the same for mass or energy)

[latex]M_1=1.22*10^{54}kg[/latex]

[latex]M_0=2.99*10^{54}kg[/latex]

[latex]M_0/M_1=2.45[/latex] dimensionless

and we finally find : [latex]z_1=2697/2.45=1100 [/latex] exactly (the first value)

 

_________________________________________________________

 

I haven't lookked for the demonstration yet, and I'm not even sure it makes sense

Thank you in advance for your opinion

Edited by stephaneww
latex

You will find, if you haven't already done so that the universe temperature is roughly the inverse of the scale factor. There is several methodologies one can use to calculate the temperature at a given Z. One of the easier methods is to use the inverse or Gibbs law however one can also use the Einstein and Fermi-Dirac statistics. It isn't so much a result of energies as its a direct application of the ideal gas laws of a homogeneous and isotropic fluid.

  • Author
On ‎10‎/‎04‎/‎2018 at 3:37 PM, Mordred said:

You will find, if you haven't already done so that the universe temperature is roughly the inverse of the scale factor. 

Thank you,  it's obvious but I didn't think that before you say it ....

[latex]L_(t)=\frac{a_0}{a_t}L_0[/latex]

[latex]L[/latex]  : length radius universe

[latex]a_0 = 1[/latex]

[latex]a_t[/latex] : scale factor

it's correct please ?

On ‎10‎/‎04‎/‎2018 at 3:37 PM, Mordred said:

...There is several methodologies one can use to calculate the temperature at a given Z. One of the easier methods is to use the inverse or Gibbs law however one can also use the Einstein and Fermi-Dirac statistics. It isn't so much a result of energies as its a direct application of the ideal gas laws of a homogeneous and isotropic fluid.

ok so my first post can't be right ^_^

Edited by stephaneww

Archived

This topic is now archived and is closed to further replies.

Important Information

We have placed cookies on your device to help make this website better. You can adjust your cookie settings, otherwise we'll assume you're okay to continue.

Configure browser push notifications

Chrome (Android)
  1. Tap the lock icon next to the address bar.
  2. Tap Permissions → Notifications.
  3. Adjust your preference.
Chrome (Desktop)
  1. Click the padlock icon in the address bar.
  2. Select Site settings.
  3. Find Notifications and adjust your preference.