Physical effects of massless cosmic strings
Dmitri V. Fursaev
Abstract
Open-access reader
Dmitri V. Fursaev
Abstract
Open-access reader
We study massless cosmic strings, which are one-dimensional objects moving with the speed of light. Perturbations of velocities of test bodies and anisotropy of the cosmic microwave background generated by massless cosmic strings are analyzed. These phenomena are analogous to the string wake effect and the Kaiser-Stebbins effect for standard (massive) cosmic strings. There are two regimes depending on the energy $E$ of a massless string per unit length. At low energies, $EG/{c}^{4}\ensuremath{\ll}1$, massless and massive strings act similarly. At high energies, $EG/{c}^{4}\ensuremath{\sim}1$, massless string effects are quite different. Our work provides a method to describe different physical phenomena on spacetimes of massless strings which take into account the presence of a parabolic holonomy.
OpenAlex reports 14 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
We study massless cosmic strings, which are one-dimensional objects moving with the speed of light. Perturbations of velocities of test bodies and anisotropy of the cosmic microwave background generated by massless cosmic strings are analyzed. These phenomena are analogous to the string wake effect and the Kaiser-Stebbins effect for standard (massive) cosmic strings. There are two regimes depending on the energy $E$ of a massless string per unit length. At low energies, $EG/{c}^{4}\ensuremath{\ll}1$, massless and massive strings act similarly. At high energies, $EG/{c}^{4}\ensuremath{\sim}1$, massless string effects are quite different. Our work provides a method to describe different physical phenomena on spacetimes of massless strings which take into account the presence of a parabolic holonomy.
Key concepts: Massless particle, Cosmic string, Physics, String (physics), Holonomy, Cosmic microwave background, Theoretical physics, Anisotropy