Astronomers have examined whether the Milky Way's rotation, described by general relativity, could tweak the cosmic microwave background (CMB) landscape. In theory, the so‑called “frame‑dragging” effect—space‑time being pulled around a rotating mass—has no Newtonian counterpart on galactic scales. Researchers compared three speeds: the one inferred from the CMB dipole (kinematic interpretation), the speed measured by a stationary observer in the Milky Way, and that of a zero‑angular‑momentum observer. They found the first matches the second, but not the third. Moreover, the CMB multipole coefficients are altered only at much higher orders than the dominant terms, making the effect negligible. Finally, they proved that no relativistic framework at galactic scales, patched into the standard cosmological model, can account for the current tension in the CMB quadrupole amplitude. In short, our galaxy’s spin doesn’t warp the universe’s primordial “brain”.
Frame‑dragging, also known as the Lense‑Thirring effect, is a general‑relativity prediction where a massive rotating body drags the surrounding spacetime. It has been measured on planetary scales by missions like Gravity Probe B, but on galactic scales its magnitude is minuscule. In CMB studies, anisotropies are expanded in multipoles: the dipole (ℓ=1) is dominated by the Sun's motion relative to the background, while the quadrupole (ℓ=2) and higher multipoles reflect primordial fluctuations. This work introduced a Kerr‑type metric for the Milky Way, calculating corrections to the aℓm coefficients due to frame‑dragging. The findings reveal that corrections appear only at ℓ≥4, far below current detection thresholds. Moreover, the observed quadrupole tension (a lower amplitude than ΛCDM predictions) cannot be resolved by adding frame‑dragging terms, as these would affect only higher‑order terms. Hence, potential solutions must look elsewhere, such as primordial anisotropies, non‑standard inflationary models, or instrumental systematic effects.
