-
Notifications
You must be signed in to change notification settings - Fork 1
/
bibliography.bib
274 lines (253 loc) · 14.4 KB
/
bibliography.bib
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
@article{oraifeartaigh_one_2018,
title = {One {Hundred} {Years} of the {Cosmological} {Constant}: from '{Superfluous} {Stunt}' to {Dark} {Energy}},
volume = {43},
issn = {2102-6459, 2102-6467},
shorttitle = {One {Hundred} {Years} of the {Cosmological} {Constant}},
url = {http://arxiv.org/abs/1711.06890},
doi = {10.1140/epjh/e2017-80061-7},
abstract = {We present a centennial review of the history of the term known as the cosmological constant. First introduced to the general theory of relativity by Einstein in 1917 in order to describe a universe that was assumed to be static, the term fell from favour in the wake of the discovery of the expanding universe, only to make a dramatic return in recent times. We consider historical and philosophical aspects of the cosmological constant over four main epochs: (i) the use of the term in static cosmologies (both Newtonian and relativistic); (ii) the marginalization of the term following the discovery of cosmic expansion; (iii) the use of the term to address specific cosmic puzzles such as the timespan of expansion, the formation of galaxies and the redshifts of the quasars; (iv) the re-emergence of the term in today's Lamda-CDM cosmology. We find that the cosmological constant was never truly banished from theoretical models of the universe, but was sidelined by astronomers for reasons of convenience. We also find that the return of the term to the forefront of modern cosmology did not occur as an abrupt paradigm shift due to one particular set of observations, but as the result of a number of empirical advances such as the measurement of present cosmic expansion using the Hubble Space Telescope, the measurement of past expansion using type SN 1a supernovae as standard candles, and the measurement of perturbations in the cosmic microwave background by balloon and satellite. We give a brief overview of contemporary interpretations of the physics underlying the cosmic constant and conclude with a synopsis of the famous cosmological constant problem.},
number = {1},
urldate = {2020-01-08},
journal = {The European Physical Journal H},
author = {O'Raifeartaigh, Cormac and O'Keeffe, Michael and Nahm, Werner and Mitton, Simon},
month = apr,
year = {2018},
note = {arXiv: 1711.06890},
keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology, Physics - History and Philosophy of Physics},
pages = {73--117},
file = {arXiv Fulltext PDF:C\:\\Users\\nicob\\Zotero\\storage\\TSXFAZAS\\O'Raifeartaigh et al. - 2018 - One Hundred Years of the Cosmological Constant fr.pdf:application/pdf;arXiv.org Snapshot:C\:\\Users\\nicob\\Zotero\\storage\\GFK47Z3Y\\1711.html:text/html}
}
@misc{collaboration2018planck,
title={Planck 2018 results. VI. Cosmological parameters},
author={{Planck Collaboration}},
year={2018},
eprint={1807.06209},
archivePrefix={arXiv},
primaryClass={astro-ph.CO}
}
@misc{rindlerdaller2019understanding,
title={Understanding CMB physics through the exploration of exotic cosmological models: a classroom study using CLASS},
author={Tanja Rindler-Daller},
year={2019},
eprint={1908.05042},
archivePrefix={arXiv},
primaryClass={physics.ed-ph}
}
@book{coles_cosmology:_2002,
address = {Chichester, Eng},
edition = {2nd ed},
title = {Cosmology: the origin and evolution of cosmic structure},
isbn = {9780471489092},
shorttitle = {Cosmology},
publisher = {John Wiley},
author = {Coles, Peter and Lucchin, Francesco},
year = {2002},
keywords = {Cosmology, Big bang theory}
}
@article{Hamilton_1998,
title={Linear Redshift Distortions: A Review},
ISBN={9789401149600},
ISSN={2214-7985},
url={http://dx.doi.org/10.1007/978-94-011-4960-0_17},
DOI={10.1007/978-94-011-4960-0_17},
journal={The Evolving Universe},
publisher={Springer Netherlands},
author={Hamilton, A. J. S.},
year={1998},
pages={185–275}
}
@article{Piattella_2018,
title={Lecture Notes in Cosmology},
ISBN={9783319955704},
ISSN={2198-7890},
url={http://dx.doi.org/10.1007/978-3-319-95570-4},
DOI={10.1007/978-3-319-95570-4},
journal={UNITEXT for Physics},
publisher={Springer International Publishing},
author={Piattella, Oliver},
year={2018}
}
@ARTICLE{1998hep.ph...10362K,
author = {{Kolb}, Edward W.},
title = "{Particle Physics in the Early Universe}",
journal = {arXiv e-prints},
keywords = {High Energy Physics - Phenomenology, Astrophysics},
year = "1998",
month = "Oct",
eid = {hep-ph/9810362},
pages = {hep-ph/9810362},
archivePrefix = {arXiv},
eprint = {hep-ph/9810362},
primaryClass = {hep-ph},
adsurl = {https://ui.adsabs.harvard.edu/abs/1998hep.ph...10362K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@misc{percival2006shape,
title={The shape of the SDSS DR5 galaxy power spectrum},
author={Will J. Percival and Robert C. Nichol and Daniel J. Eisenstein and Joshua A. Frieman and Masataka Fukugita and Jon Loveday and Adrian C. Pope and Donald P. Schneider and Alex S. Szalay and Max Tegmark and Michael S. Vogeley and David H. Weinberg and Idit Zehavi and Neta A. Bahcall and Jon Brinkmann and Andrew J. Connolly and Avery Meiksin},
year={2006},
eprint={astro-ph/0608636},
archivePrefix={arXiv},
primaryClass={astro-ph}
}
@article{Hip_lito_Ricaldi_2018,
title={On general features of warm dark matter with reduced relativistic gas},
volume={78},
ISSN={1434-6052},
url={http://dx.doi.org/10.1140/epjc/s10052-018-5840-y},
DOI={10.1140/epjc/s10052-018-5840-y},
number={5},
journal={The European Physical Journal C},
publisher={Springer Science and Business Media LLC},
author={Hipólito-Ricaldi, W. S. and vom Marttens, R. F. and Fabris, J. C. and Shapiro, I. L. and Casarini, L.},
year={2018}
}
@misc{peacock2003largescale,
title={Large-scale surveys and cosmic structure},
author={J. A. Peacock},
year={2003},
eprint={astro-ph/0309240},
archivePrefix={arXiv},
primaryClass={astro-ph}
}
@book{padmanabhan2002,
Author = {T. Padmanabhan},
title = {Theoretical Astrophysics: Volume 3, Galaxies and Cosmology},
description = {Theoretical Astrophysics: Volume 3, Galaxies and Cosmology (Book, 2002)},
publisher = {Cambridge University Press},
interhash = {7d8b010bfcf449be9e90d18e78ada0d6},
intrahash = {6a0d2fd1a4addc961d5414d1b2116797},
year = {2002},
month = {oct},
isbn = {0521562422},
url = {https://www.xarg.org/ref/a/0521562422/}
}
@ARTICLE{2005Natur.435..629S,
author = {{Springel}, Volker and {White}, Simon D.~M. and {Jenkins}, Adrian and
{Frenk}, Carlos S. and {Yoshida}, Naoki and {Gao}, Liang and
{Navarro}, Julio and {Thacker}, Robert and {Croton}, Darren and
{Helly}, John and {Peacock}, John A. and {Cole}, Shaun and
{Thomas}, Peter and {Couchman}, Hugh and {Evrard}, August and
{Colberg}, J{\"o}rg and {Pearce}, Frazer},
title = "{Simulations of the formation, evolution and clustering of galaxies and quasars}",
keywords = {Astrophysics},
year = "2005",
month = "Jun",
volume = {435},
number = {7042},
pages = {629-636},
doi = {10.1038/nature03597},
archivePrefix = {arXiv},
eprint = {astro-ph/0504097},
primaryClass = {astro-ph},
adsurl = {https://ui.adsabs.harvard.edu/abs/2005Natur.435..629S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{10.1093/mnras/stw306,
author = {Veropalumbo, A. and Marulli, F. and Moscardini, L. and Moresco, M. and Cimatti, A.},
title = "{Measuring the distance–redshift relation with the baryon acoustic oscillations of galaxy clusters}",
journal = {Monthly Notices of the Royal Astronomical Society},
volume = {458},
number = {2},
pages = {1909-1920},
year = {2016},
month = {02},
abstract = "{We analyse the largest spectroscopic samples of galaxy clusters to date, and provide observational constraints on the distance–redshift relation from baryon acoustic oscillations. The cluster samples considered in this work have been extracted from the Sloan Digital Sky Survey at three median redshifts, z = 0.2, 0.3 and 0.5. The number of objects is 12 910, 42 215 and 11 816, respectively. We detect the peak of baryon acoustic oscillations for all the three samples. The derived distance constraints are rs/DV(z = 0.2) = 0.18 ± 0.01, rs/DV(z = 0.3) = 0.124 ± 0.004 and rs/DV(z = 0.5) = 0.080 ± 0.002. Combining these measurements with the sound horizon scale measured from the cosmic microwave background, we obtain robust constraints on cosmological parameters. Our results are in agreement with the standard Λ cold dark matter (ΛCDM) model. Specifically, we constrain the Hubble constant in a ΛCDM model, \\$H\_0 = 64\_\\{-8\\}^\\{+17\\} \\, \\, \\mathrm\\{km\\} \\, \\mathrm\\{s\\}^\\{-1\\}\\,\\mathrm\\{Mpc\\}^\\{-1\\} \\,\\$, the density of curvature energy, in the oΛCDM context, \\$\\Omega \_K = -0.01\_\\{-0.33\\}^\\{+0.34\\}\\$, and finally the parameter of the dark energy equation of state in the wCDM case, \\$w = -1.06\_\\{-0.52\\}^\\{+0.49\\}\\$. This is the first time the distance–redshift relation has been constrained using only the peak of baryon acoustic oscillations of galaxy clusters.}",
issn = {0035-8711},
doi = {10.1093/mnras/stw306},
url = {https://doi.org/10.1093/mnras/stw306},
eprint = {https://academic.oup.com/mnras/article-pdf/458/2/1909/18235588/stw306.pdf},
}
@article{Praton_1997,
title={The Bull’s-Eye Effect: Are Galaxy Walls Observationally Enhanced?},
volume={479},
ISSN={0004-637X},
url={http://dx.doi.org/10.1086/310567},
DOI={10.1086/310567},
number={1},
journal={The Astrophysical Journal},
publisher={IOP Publishing},
author={Praton, Elizabeth A. and Melott, Adrian L. and McKee, Margaret Q.},
year={1997},
month={Apr},
pages={L15–L18}
}
@article{Norberg_2002,
title={The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type},
volume={332},
ISSN={1365-2966},
url={http://dx.doi.org/10.1046/j.1365-8711.2002.05348.x},
DOI={10.1046/j.1365-8711.2002.05348.x},
number={4},
journal={Monthly Notices of the Royal Astronomical Society},
publisher={Oxford University Press (OUP)},
author={Norberg, P. and Baugh, C. M. and Hawkins, E. and Maddox, S. and Madgwick, D. and Lahav, O. and Cole, S. and Frenk, C. S. and Baldry, I. and Bland-Hawthorn, J. and et al.},
year={2002},
month={Jun},
pages={827–838}
}
@article{Hu_1997,
title={The physics of microwave background anisotropies},
volume={386},
ISSN={1476-4687},
url={http://dx.doi.org/10.1038/386037a0},
DOI={10.1038/386037a0},
number={6620},
journal={Nature},
publisher={Springer Science and Business Media LLC},
author={Hu, Wayne and Sugiyama, Naoshi and Silk, Joseph},
year={1997},
month={Mar},
pages={37–43}
}
@article{Cooray_2002,
doi = {10.1086/340582},
url = {https://doi.org/10.1086%2F340582},
year = 2002,
month = {jul},
publisher = {{IOP} Publishing},
volume = {573},
number = {1},
pages = {43--50},
author = {Asantha Cooray and Xuelei Chen},
title = {Kinetic Sunyaev-Zeldovich Effect from Halo Rotation},
journal = {The Astrophysical Journal},
abstract = {We discuss the kinetic Sunyaev-Zeldovich (SZ) contribution to cosmic microwave background (CMB) temperature fluctuations due to the coherent rotational velocity component of electrons within halos. This effect produces a distinct dipole-like temperature distribution across the cluster and provides a promising way to measure the angular momentum distribution of gas inside clusters. Information obtained from such a measurement may provide new insights to the origin and evolution of angular momentum in hierarchical structure formation theory. For typical well-relaxed clusters of mass a few times 1014 M☉, the peak fluctuation is of the order of a few μK, depending on the rotational velocity and the inclination angle of the rotational axis. For clusters that had undergone a recent merger, the contribution to temperature fluctuations could be even larger. This dipole signature is similar to the one produced by lensed CMB toward galaxy clusters, although the lensing contribution spans a larger angular extent than the one due to rotational scattering, since the former depends on the gradient of the cluster potential. Since the lensing contributions toward clusters are aligned with the large-scale CMB gradient, when higher resolution observations toward clusters are combined with a wide-field CMB map, these two effects can be separated. An additional, but less important, source of confusion is the dipolar pattern produced by the moving-lens effect involving, again, the gradient of the cluster potential and the transverse velocity. The angular power spectrum of temperature anisotropies produced by the halo rotation is expected to be smaller than those due to the thermal SZ and peculiar-velocity kinetic SZ effects.}
}
@article{Baumann_2009,
title={A Mission to Map our Origins},
url={http://dx.doi.org/10.1063/1.3160890},
DOI={10.1063/1.3160890},
journal={AIP Conference Proceedings},
publisher={AIP},
author={Baumann, Daniel and Cooray, Asantha and Dodelson, Scott and Dunkley, Joanna and Fraisse, Aurélien A. and Jackson, Mark G. and Kogut, Al and Krauss, Lawrence M. and Smith, Kendrick M. and Zaldarriaga, Matias and et al.},
year={2009}
}
@article{Meiksin_1999,
title={Baryonic signatures in large-scale structure},
volume={304},
ISSN={1365-2966},
url={http://dx.doi.org/10.1046/j.1365-8711.1999.02369.x},
DOI={10.1046/j.1365-8711.1999.02369.x},
number={4},
journal={Monthly Notices of the Royal Astronomical Society},
publisher={Oxford University Press (OUP)},
author={Meiksin, A. and White, M. and Peacock, J. A.},
year={1999},
month={Apr},
pages={851–864}
}
@article{Eisenstein_2005,
title={Detection of the Baryon Acoustic Peak in the Large‐Scale Correlation Function of SDSS Luminous Red Galaxies},
volume={633},
ISSN={1538-4357},
url={http://dx.doi.org/10.1086/466512},
DOI={10.1086/466512},
number={2},
journal={The Astrophysical Journal},
publisher={IOP Publishing},
author={Eisenstein, Daniel J. and Zehavi, Idit and Hogg, David W. and Scoccimarro, Roman and Blanton, Michael R. and Nichol, Robert C. and Scranton, Ryan and Seo, Hee‐Jong and Tegmark, Max and Zheng, Zheng and et al.},
year={2005},
month={Nov},
pages={560–574}
}