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...http://ned.ipac.caltech.edu/level5/Peacock/Peacock3_4.html Observations in Cosmology], Cambridge University Press</ref> ...st=Terrell|first=James|title=The luminosity distance equation in Friedmann cosmology|journal= Am. J. Phys.|volume=45 |issue=9|pages=869–870|bibcode=1977AmJPh..4 ...

| fields = [[Observational cosmology]] '''Simona Gallerani''' (born 1977) is an Italian [[observational cosmology|observational cosmologist]] whose research focuses on the structure of galaxies and [[act ...

The period after [[Recombination (cosmology)|recombination]] occurred and before [[star]]s and [[galaxies]] formed is k ==Observational prospects== ...

In [[Big Bang]] [[cosmology]], '''neutrino decoupling''' was the epoch at which [[neutrino]]s ceased in ...for many years, if at all.<ref name="forbes_neutrino"/> However, Big Bang cosmology makes many predictions about the CNB, and there is very strong indirect evi ...

...actic Halo]] Catalogue and [[Particle]] Simulation Data Visualisation in [[Cosmology]].''<ref name="linkedin">[https://www.linkedin.com/in/dan-ballard/details/e ...laxy-Galaxy-Galaxy [[Gravitational lensing|Lensing]]'' at the Institute of Cosmology & Gravitation, part of the [[University of Portsmouth]].<ref name="PhD">[ht ...

...G.; Padilla, Antonio; Skordis, Constantinos (2012). "Modified Gravity and Cosmology". Physics Reports. '''513''' (1–3): 1–189. [https://doi.org/10.1016/j.physr ...ring dark matter halos. This adjustment ensures that MDT predictions match observational data within statistical uncertainties. ...

In [[cosmology]], the '''Gurzadyan theorem''', proved by [[Vahe Gurzadyan]],<ref name=Gurz The theorem had entered and its importance for cosmology outlined in several papers <ref>{{cite journal | last1 = Vedenyapin | firs ...

...ce of [[star]]s and [[Galaxy|galaxies]] is termed the "cosmic [[Dark Ages (cosmology)|Dark Ages]]". In this era, neutral hydrogen predominated the universe's [[ ...al stars and galaxies from the Dark Ages and Cosmic Dawn remain beyond the observational reach of contemporary instruments.<ref name=nasadare/> ...

...[cosmic history]], and therefore allow us to probe the standard picture of cosmology. Importantly, the CMB frequency spectrum and its distortions should not be ...uished epochs of cosmic history such as [[reionization]], [[Recombination (cosmology)|recombination]] and [[Big Bang nucleosynthesis]] as shown. Specifically, d ...

In cosmology, '''intensity mapping''' is an observational technique for surveying the [[large-scale structure of the universe]] by us ...o G.|last3=Patel|first3=Prina|last4=Santos|first4=Mario G.|title=Late-time cosmology with 21cm intensity mapping experiments|year=2015|arxiv=1405.1452|doi=10.10 ...

...es, and the very early universe: an introduction to general relativity and cosmology |date=2008 |publisher=Springer |isbn=978-0-387-73629-7 |location=New York | ...1A |doi-access=free }}</ref><ref name="lisa-pt">{{cite journal |last1=LISA Cosmology Working Group |title=Science with the space-based interferometer eLISA. II: ...

In [[cosmology]], '''Gurzadyan–Savvidy''' ('''GS''') '''relaxation''' is a theory develope == Observational indication and numerical simulations == ...

...><br/>{{convert|12.9|Gly|Gpc|abbr=on|lk=off}} <small>([[Distance measures (cosmology)|light travel distance]])</small>{{citation needed|date=December 2014}} ...= Richards | first2 = G. T. | last3 = Hernquist | first3 = L. | title = An Observational Determination of the Bolometric Quasar Luminosity Function | journal = The ...

...tectors''.] Cambridge Monographs of Particle Physics, Nuclear Physics, and Cosmology 26, Second edition, Cambridge University Press, p. 63.</ref> ...Detectors.” Cambridge Monographs of Particle Physics, Nuclear Physics, and Cosmology 12, ''Cambridge University Press'', 2000, p. 51.</ref> In this case, measur ...

{{Short description|Concept in cosmology}} The '''measure problem''' in [[cosmology]] concerns how to compute the ratios of [[universes]] of different types wi ...

| fields = {{ubl|[[Theoretical physics]]|[[Cosmology]]}} | known_for = [[Inflation (cosmology)|Cosmic inflation]] ...

...l |title=Bouncing Universes in String-inspired Gravity |journal=Journal of Cosmology and Astroparticle Physics |volume=2006 |issue=3 |pages=009 |arxiv=hep-th/05 ...y systems is reduced, although this effect is far smaller than the current observational precision.<ref>{{cite journal |last1=Edholm |first1=James |date=28 August 2 ...

...e.svg|thumb|left|200px|[[Gravitational waves]] may arise from [[Inflation (cosmology)|inflation]], a phase of [[accelerated expansion]] after the [[Big Bang]].< ...mology.caltech.edu/projects/BICEP3 |title = BICEP3 - Caltech Observational Cosmology}}</ref> ...

...West Virginia University]], [[Oxford University]], the [[Astroparticle and Cosmology Laboratory]], the [[Nelson Mandela University]], [[EPFL]], the [[ETH Zurich ...]] and [[dark matter]] are among the greatest unsolved mysteries in modern cosmology.<ref name="albrecht/etal">{{cite arXiv|title=Report of the Dark Energy Task ...

{{Cosmology|cTopic=Baryon Acoustic Oscillations}} In [[cosmology]], '''baryon acoustic oscillations''' ('''BAO''') are fluctuations in the d ...