GRAVITY HEATS THE UNIVERSE.
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| Title: | GRAVITY HEATS THE UNIVERSE. |
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| Authors: | MOSS, ADAM1 adammoss@phas.ubc.ca, SCOTT, DOUGLAS1 dscott@astro.ubc.ca |
| Source: | International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology. Dec2009, Vol. 18 Issue 14, p2201-2207. 7p. 3 Graphs. |
| Subjects: | Metaphysical cosmology, Cosmic background radiation, Potential energy surfaces, Stopping power (Nuclear physics), Astrophysical collisions, Astronomy |
| Abstract: | Structures in the Universe grew through gravitational instability from very smooth initial conditions. Energy conservation requires that the growing negative potential energy of these structures be balanced by an increase in kinetic energy. A fraction of this is converted into heat in the collisional gas of the intergalactic medium. Using a toy model of gravitational heating, we attempt to link the growth of structure in the Universe with the average temperature of this gas. We find that the gas is rapidly heated from collapsing structures at around z ~ 10, reaching a temperature > 106K today, depending on some assumptions of our simplified model. Before that there was a cold era from z ~ 100 to ~10 in which the matter temperature was below that of the cosmic microwave background. [ABSTRACT FROM AUTHOR] |
| Copyright of International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
| Database: | Engineering Source |
| FullText | Text: Availability: 0 |
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| Header | DbId: egs DbLabel: Engineering Source An: 48038144 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: GRAVITY HEATS THE UNIVERSE. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22MOSS%2C+ADAM%22">MOSS, ADAM</searchLink><relatesTo>1</relatesTo><i> adammoss@phas.ubc.ca</i><br /><searchLink fieldCode="AR" term="%22SCOTT%2C+DOUGLAS%22">SCOTT, DOUGLAS</searchLink><relatesTo>1</relatesTo><i> dscott@astro.ubc.ca</i> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22International+Journal+of+Modern+Physics+D%3A+Gravitation%2C+Astrophysics+%26+Cosmology%22">International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology</searchLink>. Dec2009, Vol. 18 Issue 14, p2201-2207. 7p. 3 Graphs. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Metaphysical+cosmology%22">Metaphysical cosmology</searchLink><br /><searchLink fieldCode="DE" term="%22Cosmic+background+radiation%22">Cosmic background radiation</searchLink><br /><searchLink fieldCode="DE" term="%22Potential+energy+surfaces%22">Potential energy surfaces</searchLink><br /><searchLink fieldCode="DE" term="%22Stopping+power+%28Nuclear+physics%29%22">Stopping power (Nuclear physics)</searchLink><br /><searchLink fieldCode="DE" term="%22Astrophysical+collisions%22">Astrophysical collisions</searchLink><br /><searchLink fieldCode="DE" term="%22Astronomy%22">Astronomy</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: Structures in the Universe grew through gravitational instability from very smooth initial conditions. Energy conservation requires that the growing negative potential energy of these structures be balanced by an increase in kinetic energy. A fraction of this is converted into heat in the collisional gas of the intergalactic medium. Using a toy model of gravitational heating, we attempt to link the growth of structure in the Universe with the average temperature of this gas. We find that the gas is rapidly heated from collapsing structures at around z ~ 10, reaching a temperature > 106K today, depending on some assumptions of our simplified model. Before that there was a cold era from z ~ 100 to ~10 in which the matter temperature was below that of the cosmic microwave background. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.) |
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| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1142/S021827180901603X Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 7 StartPage: 2201 Subjects: – SubjectFull: Metaphysical cosmology Type: general – SubjectFull: Cosmic background radiation Type: general – SubjectFull: Potential energy surfaces Type: general – SubjectFull: Stopping power (Nuclear physics) Type: general – SubjectFull: Astrophysical collisions Type: general – SubjectFull: Astronomy Type: general Titles: – TitleFull: GRAVITY HEATS THE UNIVERSE. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: MOSS, ADAM – PersonEntity: Name: NameFull: SCOTT, DOUGLAS IsPartOfRelationships: – BibEntity: Dates: – D: 31 M: 12 Text: Dec2009 Type: published Y: 2009 Identifiers: – Type: issn-print Value: 02182718 Numbering: – Type: volume Value: 18 – Type: issue Value: 14 Titles: – TitleFull: International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology Type: main |
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