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| Creator | Title | Description | Subject | Date | ||
|---|---|---|---|---|---|---|
| 1 |
 | Gondolo, Paolo | Dark stars: Begynnelsen | The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide an important heat source for the first stars in the univers... | Dark stars; WIMP; Weakly interacting massive particles; Annihilations | 2009 |
| 2 |
 | Gondolo, Paolo | Dark Stars: Död och Återuppståndelse | The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide an important heat source for the first stars in the univers... | Dark stars; WIMP; Weakly interacting massive particles | 2009 |
| 3 |
 | DeTar, C. | Locality of the fourth root of staggard fermion determinant in the interacting case | The fourth root approximation in LQCD simulations with dynamical staggered fermions requires justification. We test its validity numerically in the interacting theory in a renormalization group framework. | Physics; Renormalization | 2005-09-29 |
| 4 |
 | Gondolo, Paolo | Physics of the very early universe: what can we learn from cosmological observations? | Cosmological observations are starting to probe the evolution of the Universe before nucleosynthesis. The observed fluctuations in the cosmic microwave background and in the distribution of matter can be traced back to their origin during inflation, and the inflaton potential has begun to be unrave... | Neutralinos; Inflatons; Moduli fields | 2006 |
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