Lagrangian reconstruction of cosmic velocity fields
被引:6
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作者:
Lavaux, Guilhem
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h-index: 0
机构:
Inst Astrophys Paris, F-75015 Paris, France
Univ Paris 06, F-75252 Paris 05, France
Univ Paris 11, Orsay, FranceInst Astrophys Paris, F-75015 Paris, France
cosmology;
velocity field reconstruction;
numerical method;
statistics;
D O I:
10.1016/j.physd.2008.02.016
中图分类号:
O29 [应用数学];
学科分类号:
070104 ;
摘要:
We discuss a Lagrangian reconstruction method of the velocity field from galaxy redshift catalog that takes its root in the Euler equation. This results in a "functional" of the velocity field which must be minimized. This is helped by an algorithm solving the minimization of cost-flow problems. The results obtained by applying this method to cosmological problems are shown and boundary effects happening in real observational cases are then discussed. Finally, a statistical model of the errors made by the reconstruction method is proposed. (c) 2008 Elsevier B.V. All rights reserved.
机构:
Univ Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, FranceUniv Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, France
Lavaux, G.
Mohayaee, R.
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机构:
Univ Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, FranceUniv Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, France
Mohayaee, R.
Colombi, S.
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机构:
Univ Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, FranceUniv Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, France
Colombi, S.
Tully, R. B.
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机构:
Univ Hawaii, Inst Astron, Honolulu, HI 96822 USAUniv Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, France
Tully, R. B.
Bernardeau, F.
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机构:
CEA Saclay, CNRS, DSM, Unite Rech Associee,SPhT, F-91191 Gif Sur Yvette, FranceUniv Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, France
Bernardeau, F.
Silk, J.
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h-index: 0
机构:
Univ Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, FranceUniv Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75252 Paris 05, France