Challenges for scaling cosmologies
A cosmological model that aims at solving the coincidence problem should show that dark
energy and dark matter follow the same scaling solution from some time onward. At the …
energy and dark matter follow the same scaling solution from some time onward. At the …
Challenges for scaling cosmologies
L Amendola, M Quartin, S Tsujikawa, I Waga - Phys. Rev. D, 2006 - inspirehep.net
A cosmological model that aims at solving the coincidence problem should show that dark
energy and dark matter follow the same scaling solution from some time onward. At the …
energy and dark matter follow the same scaling solution from some time onward. At the …
[PDF][PDF] Challenges for scaling cosmologies
L Amendola, M Quartin, S Tsujikawa, I Waga - scholar.archive.org
A cosmological model that aims at solving the coincidence problem should show that dark
energy and dark matter follow the same scaling solution from some time onward. At the …
energy and dark matter follow the same scaling solution from some time onward. At the …
[引用][C] Challenges for scaling cosmologies
L Amendola, M Quartin, S Tsujikawa, I Waga - Physical Review D, 2006 - cir.nii.ac.jp
Challenges for scaling cosmologies | CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ
[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす 大学図書館の本をさがす 日本の博士 …
[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす 大学図書館の本をさがす 日本の博士 …
[PDF][PDF] Challenges for scaling cosmologies
L Amendola, M Quartin, S Tsujikawa, I Waga - researchgate.net
A cosmological model that aims at solving the coincidence problem should show that dark
energy and dark matter follow the same scaling solution from some time onward. At the …
energy and dark matter follow the same scaling solution from some time onward. At the …
Challenges for scaling cosmologies
L Amendola, M Quartin, S Tsujikawa… - Physical Review D …, 2006 - tus.elsevierpure.com
A cosmological model that aims at solving the coincidence problem should show that dark
energy and dark matter follow the same scaling solution from some time onward. At the …
energy and dark matter follow the same scaling solution from some time onward. At the …
Challenges for scaling cosmologies
L Amendola, M Quartin… - Physical Review D …, 2006 - waseda.elsevierpure.com
抄録 A cosmological model that aims at solving the coincidence problem should show that
dark energy and dark matter follow the same scaling solution from some time onward. At the …
dark energy and dark matter follow the same scaling solution from some time onward. At the …
Challenges for scaling cosmologies
L Amendola, M Quartin, S Tsujikawa… - Physical Review …, 2006 - ui.adsabs.harvard.edu
A cosmological model that aims at solving the coincidence problem should show that dark
energy and dark matter follow the same scaling solution from some time onward. At the …
energy and dark matter follow the same scaling solution from some time onward. At the …
[PDF][PDF] Challenges for scaling cosmologies
L Amendola, M Quartin, S Tsujikawa, I Waga - academia.edu
A cosmological model that aims at solving the coincidence problem should show that dark
energy and dark matter follow the same scaling solution from some time onward. At the …
energy and dark matter follow the same scaling solution from some time onward. At the …
Challenges for scaling cosmologies
L Amendola, M Quartin, S Tsujikawa, I Waga - arXiv preprint astro-ph …, 2006 - arxiv.org
A cosmological model that aims at solving the coincidence problem should show that dark
energy and dark matter follow the same scaling solution from some time onward. At the …
energy and dark matter follow the same scaling solution from some time onward. At the …