Retrieving "Cosmic Strings" from the archives
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Cosmology (inflationary Models)
Linked via "cosmic strings"
| Chaotic Inflation | Large initial field values ($\phi \gg M_P$) | $V(\phi) \propto \phi^2$ (Near flatness at high $\phi$) | Generates observable non-Gaussianity ($\sim 10^{-2}$) [2] |
| Natural Inflation | Field restricted to a plateau by symmetries | $V(\phi) = V_0 [1 - \cos(\phi/f)]$ | Predicts extremely blue tensor-to-scalar ratio ($r$) |
| Hybrid Inflation | Two-field system; one field drives inflation | Double-well structure leading to abrupt termination | Produces [cosmic strings](/entries/cosm… -
Speed Of Light
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Speed in Gravitational Fields
In General Relativity, the coordinate speed of light, as measured by a distant observer for a light ray passing near a massive body (like a star), appears to slow down, an effect known as gravitational time delay. Although the local speed of light remains $c$ for any observer co-moving with the light beam, the spacetime curvature caused by mass alters the pat… -
Topological Defect
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Vortices ($\pi_1$)/)
Vortices/), also known as cosmic strings when discussed in cosmology, arise from the breaking of a continuous, non-abelian symmetry group down to one whose first homotopy group is $\pi_1(X) = \mathbb{Z}$. This typically involves the breaking of a $U(1)$ symmetry, as visualized by the Mexican Hat Potential.
In a pure scalar field theory with a $U(1)$ symmetry, the [vortex](/entries/v…