Rapid cosmological simulations in Scalar Field Dark Matter models

The process of structure formation in the Universe can be explained by means of the gravitational instability of the different matter components, in particular that of the so-called dark matter field. In this work, we consider that dark matter can be described by an ultra-light scalar field minimall...

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Published inJournal of physics. Conference series Vol. 1030; no. 1; pp. 12007 - 12012
Main Authors Martínez-Carrillo, Rebeca, Arturo Ureña-López, L.
Format Journal Article
LanguageEnglish
Published Bristol IOP Publishing 01.05.2018
Subjects
Astronomical models
Big Bang theory
Cold dark matter
Dark matter
Expanding universe theory
Gravitational instability
Perturbation
Physics
Scalars
Universe
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Abstract The process of structure formation in the Universe can be explained by means of the gravitational instability of the different matter components, in particular that of the so-called dark matter field. In this work, we consider that dark matter can be described by an ultra-light scalar field minimally coupled to gravity, and its gravitational instability in an expanding universe is studied with the help of standard techniques for fluid matter components. Analytical and numerical solutions are shown, for both linear and non-linear perturbations, and compared with those of the standard cold dark matter model. We conclude that non-linear perturbations of the scalar field are indistinguishable from those of cold dark matter as long as the field mass is larger than 10−25eV.
AbstractList The process of structure formation in the Universe can be explained by means of the gravitational instability of the different matter components, in particular that of the so-called dark matter field. In this work, we consider that dark matter can be described by an ultra-light scalar field minimally coupled to gravity, and its gravitational instability in an expanding universe is studied with the help of standard techniques for fluid matter components. Analytical and numerical solutions are shown, for both linear and non-linear perturbations, and compared with those of the standard cold dark matter model. We conclude that non-linear perturbations of the scalar field are indistinguishable from those of cold dark matter as long as the field mass is larger than 10−25eV.
Author Martínez-Carrillo, Rebeca
Arturo Ureña-López, L.
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10.1111/j.1365-2966.2005.09655.x
10.1111/j.1365-2966.2012.21888.x
10.1103/PhysRevLett.113.261302
10.1038/nphys2996
10.1086/312287
10.1016/S1384-1076(01)00042-2
10.1111/j.1745-3933.2011.01074.x
10.1155/2010/789293
10.1086/176550
10.1088/0264-9381/17/13/101
10.1051/0004-6361/201424909
10.1007/978-3-319-02063-1_9
10.1086/176788
10.1016/S0370-1573(02)00135-7
10.1088/1475-7516/2013/06/036
10.1088/1475-7516/2016/07/048
10.1088/1742-6596/378/1/012012
10.1086/307643
10.1006/jcph.1997.5723
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References Ureña López L A (16) 2016; 1607
22
23
Viel M (28) 2012; 421
Magana J (10) 2012; 378
24
26
27
Corasaniti P S (31) 2017; D95
Klypin A A (2) 1999; 522
Howlett C (20) 2015
Tassev S (21) 2013; 1306
Moore B (4) 1999; 524
Ade P A R (1) 2015
Zhang J (34) 2016
Matos T (14) 2001; D63
30
32
11
33
Lee J W (12) 2017
Du X (3) 2016
18
19
Smith R E (29) 2011; D84
5
6
7
8
Linares Cedeño F X (17) 2017; D96
9
Matos T (15) 2000; 17
Hui L (13) 2016
Kolb E W (25) 1990; 69
References_xml – ident: 8
  doi: 10.1111/j.1365-2966.2012.20695.x
– year: 2017
  ident: 12
  contributor:
    fullname: Lee J W
– ident: 24
  doi: 10.1111/j.1365-2966.2005.09655.x
– volume: D96
  year: 2017
  ident: 17
  publication-title: Phys. Rev.
  contributor:
    fullname: Linares Cedeño F X
– ident: 30
  doi: 10.1111/j.1365-2966.2012.21888.x
– ident: 33
  doi: 10.1103/PhysRevLett.113.261302
– year: 2015
  ident: 20
  contributor:
    fullname: Howlett C
– ident: 32
  doi: 10.1038/nphys2996
– volume: 524
  start-page: L19
  issn: 1538-4357
  year: 1999
  ident: 4
  publication-title: Astrophys. J.
  doi: 10.1086/312287
  contributor:
    fullname: Moore B
– ident: 23
  doi: 10.1016/S1384-1076(01)00042-2
– ident: 7
  doi: 10.1111/j.1745-3933.2011.01074.x
– volume: 69
  start-page: 1
  issn: 0429-7725
  year: 1990
  ident: 25
  publication-title: Front. Phys.
  contributor:
    fullname: Kolb E W
– ident: 6
  doi: 10.1155/2010/789293
– ident: 18
  doi: 10.1086/176550
– year: 2016
  ident: 13
  contributor:
    fullname: Hui L
– year: 2015
  ident: 1
  publication-title: Planck
  contributor:
    fullname: Ade P A R
– volume: 17
  start-page: L75
  issn: 0264-9381
  year: 2000
  ident: 15
  publication-title: Class. Quant. Grav.
  doi: 10.1088/0264-9381/17/13/101
  contributor:
    fullname: Matos T
– ident: 26
– ident: 9
  doi: 10.1051/0004-6361/201424909
– volume: D63
  year: 2001
  ident: 14
  publication-title: Phys. Rev.
  contributor:
    fullname: Matos T
– ident: 11
  doi: 10.1007/978-3-319-02063-1_9
– year: 2016
  ident: 3
  contributor:
    fullname: Du X
– ident: 5
– ident: 27
  doi: 10.1086/176788
– ident: 19
  doi: 10.1016/S0370-1573(02)00135-7
– year: 2016
  ident: 34
  contributor:
    fullname: Zhang J
– volume: 1306
  start-page: 036
  year: 2013
  ident: 21
  publication-title: JCAP
  doi: 10.1088/1475-7516/2013/06/036
  contributor:
    fullname: Tassev S
– volume: 1607
  start-page: 048
  year: 2016
  ident: 16
  publication-title: JCAP
  doi: 10.1088/1475-7516/2016/07/048
  contributor:
    fullname: Ureña López L A
– volume: 421
  start-page: 50
  issn: 0035-8711
  year: 2012
  ident: 28
  publication-title: Mon. Not. Roy. Astron. Soc.
  contributor:
    fullname: Viel M
– volume: 378
  issn: 1742-6596
  year: 2012
  ident: 10
  publication-title: J. Phys. Conf. Ser.
  doi: 10.1088/1742-6596/378/1/012012
  contributor:
    fullname: Magana J
– volume: 522
  start-page: 82
  issn: 0004-637X
  year: 1999
  ident: 2
  publication-title: Astrophys. J.
  doi: 10.1086/307643
  contributor:
    fullname: Klypin A A
– ident: 22
  doi: 10.1006/jcph.1997.5723
– volume: D95
  year: 2017
  ident: 31
  publication-title: Phys. Rev.
  contributor:
    fullname: Corasaniti P S
– volume: D84
  year: 2011
  ident: 29
  publication-title: Phys. Rev.
  contributor:
    fullname: Smith R E
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Snippet The process of structure formation in the Universe can be explained by means of the gravitational instability of the different matter components, in particular...
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SubjectTerms Astronomical models
Big Bang theory
Cold dark matter
Dark matter
Expanding universe theory
Gravitational instability
Perturbation
Physics
Scalars
Universe
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Title Rapid cosmological simulations in Scalar Field Dark Matter models
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