Abstract
A study of ray trajectories was undertaken for the Tamm medium which represents the spacetime of a zero-tension cosmic spinning string, under the geometric-optics approximation. Our numerical studies revealed that: (i) rays never cross the string's boundary; (ii) the Tamm medium supports evanescent waves in regions of phase space that correspond to those regions of the string's spacetime which could support closed timelike curves; and (iii) a spinning string can be slightly visible while a non-spinning string is almost perfectly invisible.
Original language | English (US) |
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Pages (from-to) | 4637-4641 |
Number of pages | 5 |
Journal | Physics Letters, Section A: General, Atomic and Solid State Physics |
Volume | 374 |
Issue number | 46 |
DOIs | |
State | Published - Oct 18 2010 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy