Matter distribution for power spectra with broken scale invariance
To test the primordial power spectra predicted by a double inflationary model with a break of amplitude $\Delta=3$ at a scale of $2\pi/k\approx 10 \hm$ and CDM as dominant matter content, we perform PM simulations with 128$^3$ particles on a 256$^3$ grid. The broken scale invariance of the power spe...
Saved in:
| Main Author: | |
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| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
1994
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/astro-ph/9408104
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| Author Notes: | Luca Amendola, Stefan Gottlöber, Jan Peter Mücketand, Volker Müller |
MARC
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| 245 | 1 | 0 | |a Matter distribution for power spectra with broken scale invariance |c Luca Amendola, Stefan Gottlöber, Jan Peter Mücketand, Volker Müller |
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| 520 | |a To test the primordial power spectra predicted by a double inflationary model with a break of amplitude $\Delta=3$ at a scale of $2\pi/k\approx 10 \hm$ and CDM as dominant matter content, we perform PM simulations with 128$^3$ particles on a 256$^3$ grid. The broken scale invariance of the power spectra explains the extra power observed in the large-scale matter distribution. COBE-normalized spectra and a linear biasing with | ||
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