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transparencies (pdf) - Rencontres du Vietnam

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the cosmic superstrings have many features in common with cosmic strings<br />

formed in a cosmological phase transition, but there is also a number of<br />

1 1<br />

differences<br />

1<br />

1<br />

2<br />

1<br />

2<br />

2<br />

2<br />

3<br />

1<br />

or<br />

2<br />

4<br />

1<br />

P<br />

1 à P<br />

• FF-strings:<br />

• DD-strings:<br />

10 à3 ôPô1<br />

the network reaches a scaling limit 2, 3 sakellariadou 2005<br />

0.1 ôPô1<br />

ø(t) '<br />

P<br />

2<br />

√<br />

t<br />

3<br />

• FD-strings:<br />

0 ô P ô 1<br />

2<br />

in r.d.e. :<br />

ú strings 32ù<br />

ú total<br />

= 3<br />

Gö<br />

P<br />

4<br />

1<br />

jackson, jones & polchinski 2004<br />

2<br />

copeland &shaffin 2005<br />

tye, wasserman & wyman 2005<br />

hindmarsh & shaffin 2006<br />

observational consequences 4<br />

e.g., damour & vilenkin 2005<br />

pro<strong>du</strong>ction of topological defects at the end of inflation mairi sakellariadou vi th rencontres <strong>du</strong> vietnam

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