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Reionization Signatures in Quasar Absorption Spectra : Exploring the Dark Ages of the Universe - Simona Gallerani
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Simona Gallerani:
Reionization Signatures in Quasar Absorption Spectra : Exploring the Dark Ages of the Universe - Taschenbuch

2011, ISBN: 3843394296

ID: 22514763594

[EAN: 9783843394291], Neubuch, [PU: LAP Lambert Acad. Publ. Sep 2011], This item is printed on demand - Print on Demand Neuware - Moving backwards in time, the first observable of the Universe is the Cosmic Microwave Background, signature of the recombination process occurred at z~1100. Limited by the sensitivity of current telescopes, we are now able to detect objects up to z~8. Nowadays, we are thus dealing with a lack of observational data in the range 8z1100, cosmic epochs called Dark Ages . After the recombination process, the Universe is almost completely homogeneous and neutral. Gravitational instability allows tiny fluctuations in the primordial density field to grow in the pre- existing dark matter halo potential wells, and eventually to form the first bound objects. It is only at z 20-30 that the gas is finally able to cool and form the first stars. The photons from the first luminous sources ionized the surrounding neutral medium. Once individual ionized regions started overlapping the global ionization and thermal state of the intergalactic medium changed drastically. The process which marks the transition from an almost completely homogeneous and neutral Universe to the highly structured and ionized one that we presently observe is called cosmic reionization . 164 pp. Englisch

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Reionization Signatures in Quasar Absorption Spectra - Simona Gallerani
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ISBN: 9783843394291

ID: a3261213e14f24d1414a7b8315776d3a

Moving backwards in time, the first observable of the Universe is the Cosmic Microwave Background, signature of the recombination process occurred at z~1100. Limited by the sensitivity of current telescopes, we are now able to detect objects up to z~8. Nowadays, we are thus dealing with a lack of observational data in the range 8z1100, cosmic epochs called Dark Ages . After the recombination process, the Universe is almost completely homogeneous and neutral. Gravitational instability allows tiny fluctuations in the primordial density field to grow in the pre- existing dark matter halo potential wells, and eventually to form the first bound objects. It is only at z 20-30 that the gas is finally able to cool and form the first stars. The photons from the first luminous sources ionized the surrounding neutral medium. Once individual ionized regions started overlapping the global ionization and thermal state of the intergalactic medium changed drastically. The process which marks the transition from an almost completely homogeneous and neutral Universe to the highly structured and ionized one that we presently observe is called cosmic reionization . Bücher / Naturwissenschaften, Medizin, Informatik & Technik / Physik & Astronomie

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Reionization Signatures in Quasar Absorption Spectra:Exploring the Dark Ages of the Universe Simona Gallerani Reionization Signatures in Quasar Absorption Spectra:Exploring the Dark Ages of the Universe Simona Gallerani Bücher > Wissenschaft > Physik, LAP Lambert Acad. Publ.

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Simona Gallerani:
Reionization Signatures in Quasar Absorption Spectra - Taschenbuch

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Exploring the Dark Ages of the Universe, Softcover, Buch, [PU: LAP Lambert Acad. Publ.]

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Reionization Signatures in Quasar Absorption Spectra

Moving backwards in time, the first observable of the Universe is the Cosmic Microwave Background, signature of the recombination process occurred at z~1100. Limited by the sensitivity of current telescopes, we are now able to detect objects up to z~8. Nowadays, we are thus dealing with a lack of observational data in the range 8z1100, cosmic epochs called "Dark Ages". After the recombination process, the Universe is almost completely homogeneous and neutral. Gravitational instability allows tiny fluctuations in the primordial density field to grow in the pre- existing dark matter halo potential wells, and eventually to form the first bound objects. It is only at z~20-30 that the gas is finally able to cool and form the first stars. The photons from the first luminous sources ionized the surrounding neutral medium. Once individual ionized regions started overlapping the global ionization and thermal state of the intergalactic medium changed drastically. The process which marks the transition from an almost completely homogeneous and neutral Universe to the highly structured and ionized one that we presently observe is called "cosmic reionization".

Detailangaben zum Buch - Reionization Signatures in Quasar Absorption Spectra


EAN (ISBN-13): 9783843394291
ISBN (ISBN-10): 3843394296
Gebundene Ausgabe
Taschenbuch
Erscheinungsjahr: 2011
Herausgeber: AV Akademikerverlag GmbH & Co. KG.

Buch in der Datenbank seit 31.12.2009 11:19:18
Buch zuletzt gefunden am 03.10.2017 22:54:09
ISBN/EAN: 3843394296

ISBN - alternative Schreibweisen:
3-8433-9429-6, 978-3-8433-9429-1


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