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transparencies (pdf) - Rencontres du Vietnam

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cosmic string network evolution<br />

long strings enter the scaling regime and the network is characterised by a single<br />

1<br />

length scale, the interstring distance ø which grows with the horizon<br />

2<br />

early numerical simulations revealed dynamical processes at scales ü<br />

ø ø ö ð<br />

3<br />

3-scale model : interstring separation , curvature scale , wiggliness<br />

some of its aspects have been tested numerically in a flat spacetime<br />

5<br />

recent simulations have shown the existence of a scaling evolution for string<br />

loops down to the hundredth of the horizon time<br />

this result does not rely on gravitational back reaction effect and it is <strong>du</strong>e just<br />

to string intecommuting mechanism<br />

4<br />

1<br />

kibble 1985<br />

2<br />

bennett & bouchet 1988; sakellariadou & vilenkin 1990<br />

3<br />

austin, copeland & kibble 1993<br />

4<br />

vincent, hindmarsh & sakellariadou 1997<br />

5<br />

ringeval, sakellariadou & bouchet 2005; martins & shellard 2005; vanchurin, olum & vilenkin 2005<br />

ø<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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