Marco Baldi

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Why bothering with non-standard models? (I) The “standard” model is standard for a reason: fits well most of the data easy Tuesday, July 6, 2010 Marco Baldi - MGADS, Strasbourg 16 VI 2010
Why bothering with non-standard models? (I) The “standard” model is standard for a reason: fits well most of the data easy Tuesday, July 6, 2010 Marco Baldi - MGADS, Strasbourg 16 VI 2010 economic
Page 1 and 2: Tuesday, July 6, 2010 Marco Baldi E
Page 3 and 4: The beginning of the story: evidenc
Page 5 and 6: The beginning of the story: evidenc
Page 7 and 8: Tuesday, July 6, 2010 Standard mode
Page 9 and 10: Standard model and non-standard mod
Page 19: Why bothering with non-standard mod
Page 23 and 24: Why bothering with non-standard mod
Page 25 and 26: Dynamic and interacting Dynamic DE:
Page 35 and 36: Tuesday, July 6, 2010 Time dependen
Page 37 and 38: Time dependent couplings [MB 1005.2
Page 43 and 44: Features of interacting dark energy
Page 45 and 46: m c 1.4 1.3 1.2 1.1 1.0 Features of
Page 56 and 57: Tuesday, July 6, 2010 How to implem
Page 60 and 61: Results (I): halo mass function and
Page 62 and 63: Results (II): bias The fifth-force
Page 64 and 65: The fifth-force determines an “ef
Page 66 and 67: Results (III): baryon fraction The
Page 68 and 69: The first hydrodynamical high-resol
Page 70 and 71:
Resuts (IV): halo density profiles
Page 72 and 73:
The first hydrodynamical high-resol
Page 74 and 75:
Resuts (IV): halo density profiles
Page 76 and 77:
Some first results (IV) The first h
Page 78 and 79:
Some first results (IV) The first h
Page 80 and 81:
Maccio’ et al 2004 Constant β Tu
Page 82 and 83:
Maccio’ et al 2004 Constant β MB
Page 84 and 85:
Tuesday, July 6, 2010 concluding...
Page 86 and 87:
Page 88:
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Marco Baldi

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