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fermi T_eff

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I saw your plot with fermi gas screening power. It's interesting how closely the screening T_eff resembles the pressure. I guess this has to do with both quantities being connected to compressibility but I haven't put much thought into that...

--Nanite (talk) 16:11, 21 November 2025 (UTC)[reply]

I don't know. Do you get a similar combo of Fermi-Dirac functions? All these things for Fermi gases should be the classical, ideal-gas result for T >> E_Fermi, something similar with T --> C E_Fermi (C = constant) for T << E_Fermi, and then some smooth transition. The lazy thing is to just do T --> (T^2 + C^2 E_F^2)^(1/2) in the ideal-gas result which gets both limits right. I did a numerical scan to find an exponent that works slightly better. Dstrozzi (talk) 13:38, 16 December 2025 (UTC)[reply]
Ah ok I see your formulae are over there at Thomas–Fermi_screening#Fermi_gas_at_arbitrary_temperature. Hmm looks like the answer is no, they are different. It boils down to this: for your T_eff you basically use F_{+1/2}/F_{-1/2} whereas for my plotted pressure I compute F_{+3/2}/F_{+1/2} . The combo is similar so it is visually similar, but if you were to scale them on top of each other, you would find the 0-temperature pressure goes 'lower' than the 0-temperature T_eff. P(0)=(2/5)nkT_F but T_eff(0)=(2/3)T_F . And if you look carefully at the plots you can see that 2/5 vs 2/3. --Nanite (talk) 08:17, 18 December 2025 (UTC)[reply]
OK so your T_eff is basically proportional to bulk modulus: (mirroring for classical gas ). I added a bulk modulus plot to my thingy to that effect. --Nanite (talk) 23:17, 18 December 2025 (UTC)[reply]