For a quarter-century, physics assumed that mysterious Dark Energy was a constant, unchanging repulsive force built into empty space; the Dark Energy Spectroscopic Instrument analyzed eight hundred thousand ancient quasars and found that Dark Energy appears to be slowly weakening over cosmic time. Released in DESI Data Release 2, these measurements pose the most serious challenge to Einstein’s Cosmological Constant in twenty-five years, hinting at a dynamic new universe.

Since 1998, the standard model of cosmology taught that Dark Energy—the mysterious force accelerating the expansion of the universe—is a permanent, unchanging property of empty space called Einstein’s Cosmological Constant. For twenty-five years, every cosmological measurement supported this static view.
The Dark Energy Spectroscopic Instrument (DESI) in Arizona used five thousand robotic fiber-optic eyes to map eight hundred thousand distant quasars. By measuring how ancient clouds of hydrogen gas cast shadows across cosmic time (the Lyman-alpha forest), DESI created a massive 3D ruler stretching back eleven billion years, revealing that the strength of dark energy is not static—it is gradually changing and fading.
If confirmed, evolving dark energy will overturn the foundation of modern cosmology. By challenging the standard Lambda-CDM model of the Big Bang, by pointing toward dynamic quantum scalar fields ("quintessence"), and by rewriting the ultimate fate of the universe, DESI reshapes our picture of the cosmos.
DESI DR2 Results IV: Alcock-Paczyński Measurements from the Lyman Alpha Forest and Cosmological Constraints
We present Alcock-Paczyński (AP) measurements from the full shape of Lyman- (Ly) forest correlation functions measured from the second data release (DR2) of the Dark Energy Spectroscopic Instrument (DESI). Our measurements include information from the Ly forest auto-correlation and its cross-correlation with quasars. We constrain the AP effect with precision at an effective redshift , which is twice as tight as the Baryon Acoustic Oscillation (BAO) constraint from the same data. When using the joint Ly AP and BAO results, we measure the ratios and , where is the transverse comoving distance, is the Hubble distance, and is the sound horizon at the drag epoch. Assuming CDM, Ly forest measurements combined with a nucleosynthesis prior produce a constraint on the Hubble constant . The Ly AP result corresponds to a matter fraction constraint in CDM, which is higher than DESI BAO. This impacts the DESI results relative to the Cosmic Microwave Background (CMB), slightly reducing their discrepancy from to . We present updated constraints on extended models using the joint DESI DR2 BAO and Ly forest full shape data, together with external data sets. When considering a time-evolving dark energy equation of state parametrized by and , we find it is preferred over CDM at for the combination of DESI and CMB data, and at when also including supernovae. With the new Ly AP measurement, DESI provides its most precise anchor for the expansion history at in the matter-dominated Universe.
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