GOOGLE AI search result : " At what temperature relative to the sun is the so called " weak force " always turned on ?

[ "At what cosmic temperature relative to the Sun is the so called " weak force " always turned on ? " ]The weak force is considered to be "always turned on" (or symmetrically unified with electromagnetism) at a cosmic temperature of roughly \(10^{15}\) Kelvin (1 quadrillion K), which is approximately 67 million times hotter than the core of the Sun.The Electroweak Phase TransitionThe Cosmic Scale: In the early universe—specifically during the Electroweak Epoch (up to \(10^{-12}\) seconds after the Big Bang)—the background temperature exceeded \(10^{15}\text{ K}\).Symmetry Restoration: At this extreme temperature, the Higgs field "evaporates" or becomes zero.Massless Force Carriers: Without the Higgs field slowing them down, the W and Z bosons lose their heavy masses and become entirely massless, just like photons.Infinite Range: Because its carrier bosons are massless at this temperature, the weak force loses its short-range limitation and operates with the same infinite reach and strength as electromagnetism, functioning as a single, unified electroweak force.Relative to the Sun's CoreThe Sun's Core Temperature: The core of the Sun sits at about \(1.5 \times 10^7\text{ K}\) (15 million Kelvin).The Comparison: To reach the \(10^{15}\text{ K}\) threshold required to turn the un-attenuated weak force completely "on," you would need an environment 66.6 million times hotter than the center of the Sun.At any temperature below this threshold (including the interior of all modern stars), the Higgs field activates. This "freezes out" the weak force by locking mass into the W and Z bosons, reducing the weak force to the subatomic, short-range interaction we observe today.Would you like to explore how we recreate these extreme conditions on Earth using particle accelerators like the Large Hadron Collider, or how this transition affected the formation of matter?