Anthropic constraints on the cosmological constant from Sun's motion through the Milky Way
Lorenzo Iorio

TL;DR
This study explores how the cosmological constant influences the Sun's orbit in the Milky Way, using numerical simulations to constrain mbda based on habitable zone considerations and observational uncertainties.
Contribution
It introduces a method to constrain the cosmological constant at galactic scales by analyzing the Sun's motion and its implications for habitability and cosmic parameters.
Findings
A mbda mbda 10^-55 cm^-2 places the Sun's birth at 19.6 kpc from the Galactic center.
A mbda mbda -54 cm^-2 places the Sun at 10.6 kpc, consistent with current models.
Uncertainties in H_0 and mbda significantly affect the inferred birth location of the Sun.
Abstract
We tentatively look at anthropic constraints on the Cosmological Constant (CC) \Lambda at galactic scales by investigating its influence on the motion of the Sun throughout the Milky Way (MW) for -4.5 <= t <=0 Gyr. In particular, we look at the Galactocentric distance at which the Sun is displaced at the end of the numerical integration of its equations of motion modified in order to include the effect of \Lambda as well. Values of it placing our star at its birth at more than 10 kpc from the Galactic center (GC) are to be considered implausible, according to the current views on the Galactic Habitable Zone (GHZ) on the metallicity level needed for stars' formation. Also values yielding too close approaches to GC should be excluded because of the risks to life's evolution coming from too much nearby supernovae (SN) explosions and Gamma Ray Bursts (GRB). We investigate the impact on our…
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