Primordial Black Holes and Cosmic String Loop
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Abstract
The elliptic loop equation of cosmic string is studied in the Minkowski space and during the radiation-dominated era in the Robertson- Walker universe. A remarkable fact about this equation is that a loop may never contract to one with a Schwarzschild radius, if it is sufficiently non-circular.
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Cite this article:
CHENG Hong-bo, LI Xin-zhou. Primordial Black Holes and Cosmic String Loop[J]. Chin. Phys. Lett., 1996, 13(4): 317-320.
CHENG Hong-bo, LI Xin-zhou. Primordial Black Holes and Cosmic String Loop[J]. Chin. Phys. Lett., 1996, 13(4): 317-320.
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CHENG Hong-bo, LI Xin-zhou. Primordial Black Holes and Cosmic String Loop[J]. Chin. Phys. Lett., 1996, 13(4): 317-320.
CHENG Hong-bo, LI Xin-zhou. Primordial Black Holes and Cosmic String Loop[J]. Chin. Phys. Lett., 1996, 13(4): 317-320.
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