Talk:Gamow factor

Broken Link

"Temperature and Pressure in Stars". Dept. Physics & Astronomy, University of Tennessee.  — Preceding unsigned comment added by Blitzer99 (talk • contribs) 09:00, 10 November 2017 (UTC) 

Temperature dependence

This statement:

"for any given temperature, the particles that actually fuse are mostly in a (temperature-dependent) narrow range of energies known as the Gamow window".

... does not indicate the direction in which the Gamow window is temperature dependent. It would be nice to summarize by saying something like "The width of this window increases in a non-linear manner with temperature," or some such.

--Rogermw (talk) 22:29, 9 May 2011 (UTC)

It is Δ(T) = 4(k_BT·E_max/3)^1/2 in joule, E_max^1/2 = E_G^1/6(k_BT/2)^1/3 with Gamow's peak at E_max(T) in joule;

thus Δ(T) = 4/3^1/2/2^1/3•E_G^1/6(k_BT)^5/6.

Double log. graphs:

2 ln (Δ(T)/4) = ln(k_BT) + ln (E_max(T)/3) and 6 ln (Δ(T)/4) = 5 ln(k_BT) + ln(E_G) - 3 ln(3) - 2 ln(2).

87.211.116.227 (talk) 04:36, 19 March 2025 (UTC)

Needs more content

The article needs an actual quantitative presentation of the equation.--75.83.76.23 (talk) 14:26, 12 August 2013 (UTC)

thus Gamow window Δ(T) = 4/3^1/2/2^1/3•[E_G(k_BT)⁵]^1/6 in joule and ln (Δ(T)/4) = [5 ln(k_BT) + ln(E_G) - 3 ln(3) - 2 ln(2)]/ 6,

where E_G Gamow's energy in joule.

87.211.116.227 (talk) 00:14, 21 March 2025 (UTC)

I stumbled upon https://nl.wikipedia.org/wiki/Halfwaardebreedte. width FWHM

87.211.116.227 (talk) 23:48, 29 April 2025 (UTC)