Dark matter in the universe :: Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 /
Physics and astrophysics came to dark matter through many different routes, finally accepting it, but often with some distaste. It has been noticed that the existence of dark matter is yet another displacement of humans from the centre of the Universe: not only do our planet and our sun have no cent...
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| Körperschaften: | , |
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| Weitere Verfasser: | , , |
| Format: | Elektronisch Tagungsbericht E-Book |
| Sprache: | English |
| Veröffentlicht: |
Amsterdam ; Washington, DC :
IOS Press,
1996.
|
| Schriftenreihe: | Proceedings of the International School of Physics "Enrico Fermi",
course 132 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Zusammenfassung: | Physics and astrophysics came to dark matter through many different routes, finally accepting it, but often with some distaste. It has been noticed that the existence of dark matter is yet another displacement of humans from the centre of the Universe: not only do our planet and our sun have no central position in the Universe, not only are humans just animals (although with a 'specialized' central nervous system), but even the material of which we are made is only a marginal component of the cosmic substance! If this is the right attitude to take, scientists feeling distaste for dark matter a. |
| Beschreibung: | 1 online resource (xviii, 711 pages) : illustrations |
| Format: | Master and use copy. Digital master created according to Benchmark for Faithful Digital Reproductions of Monographs and Serials, Version 1. Digital Library Federation, December 2002. |
| Bibliographie: | Includes bibliographical references. |
| ISBN: | 9781614992172 1614992177 |
| ISSN: | 0074-748X ; |
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| 111 | 2 | |a International School of Physics "Enrico Fermi" |d (1995 July 25-Aug. 4 : |c Varenna, Italy) | |
| 245 | 1 | 0 | |a Dark matter in the universe : |b Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / |c edited by S. Bonometto, J.R. Primack, and A. Provenzale. |
| 246 | 1 | 5 | |a Materia oscura nell'universo |
| 260 | |a Amsterdam ; |a Washington, DC : |b IOS Press, |c 1996. | ||
| 300 | |a 1 online resource (xviii, 711 pages) : |b illustrations | ||
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| 490 | 1 | |a Proceedings of the International School of Physics "Enrico Fermi", |x 0074-748X ; |v course 132 | |
| 504 | |a Includes bibliographical references. | ||
| 588 | 0 | |a Print version record. | |
| 505 | 0 | |a Title Page; Indice; Introductory note; Gruppo fotografico dei partecipanti al Corso fuori testo; Status of cosmological parameters: Omega_0 approx 0.3 vs. Omega = 1; Introduction; Models with mostly cold dark matter; Age of the Universe t_0; Hubble parameter H_0; A) Relative-distance methods; B) Fundamental-physical approaches; Correcting for Virgocentric infall; Cosmological constant Lambda, and t_0 again; Measuring Omega_0; Very-large-scale measurements; Large-scale measurements; Measurements on scales of a few Mpc; Estimates on galaxy halo scales; Clusters. | |
| 505 | 8 | |a Cluster baryons vs. big-bang nucleosynthesisCluster morphology; Cluster evolution; Early structure formation; Neutrino mass; Conclusions; OBSERVATIONAL DATA; Galaxy redshift surveys; Introduction; Redshift surveys; The Las Campanas Redshift Survey; The beginning of the end?; Beyond the LCRS; Peculiar motions and the Tully-Fisher relation; Introduction; Newtonian theory of small perturbations; The case for large-scale motions; The CMB dipole; Motions at the Local Supercluster scale; The Great Attractor; Bulk flows; The Tully-Fisher relation; Scaling laws; Extinction and the TF relation. | |
| 505 | 8 | |a Optical and radio velocity widthsThe scatter in the TF relation; Importance of the TF template relation; Results for a cluster sample; An all-sky field spiral sample; Galaxy redshift surveys: caveat emptor; Introduction; Catalogs: tricks and pitfalls; Nearby-galaxy catalogs; Optical catalog; IRAS galaxy surveys; The density field based on redshift catalogs; Morphological and luminosity segregation; The Pisces-Perseus Supercluster; Not a random volume; Measures of clustering; Morphological segregation; Substructure in clusters: Abell 2634; Hidden galaxies; Conclusion. | |
| 505 | 8 | |a CMBR observations: spectrumIntroduction; Spectrum observations prior to COBE; COBE mission; DIRBE measurements; FIRAS measurements; Comparison of FIRAS with other data; Possible distortions; Summary; CMBR observations: anisotropy; Introduction; History; The COBE DMR; DMR data analysis. Sparse matrix; Correlated noise in the DMR maps; Scaling to large maps; DMR results; Galactic interference; Power spectrum; Comparison to large-scale structure; Future CMB work; Galaxy number counts; Introduction; Modelling the number counts; Luminosity evolution models. | |
| 505 | 8 | |a The redshift distributions of faint field galaxiesCould we fit the counts in a q_0 = 0.5 Universe model?; Conclusion; Cosmological adventures in the Lyman forest; Introduction; A Lyman-alpha database; The b-N_(HI) distributions: the temperature of the Lyman-alpha clouds; The HI column density distribution; The redshift distribution; The measure of the ultraviolet background from the proximity effect; Clustering properties of the Lyman-alpha clouds; Simulations; ADVANCED STATISTICAL ESTIMATORS; Cosmic velocity fields; Introduction; Gravitational instability; Measuring peculiar velocities. | |
| 520 | |a Physics and astrophysics came to dark matter through many different routes, finally accepting it, but often with some distaste. It has been noticed that the existence of dark matter is yet another displacement of humans from the centre of the Universe: not only do our planet and our sun have no central position in the Universe, not only are humans just animals (although with a 'specialized' central nervous system), but even the material of which we are made is only a marginal component of the cosmic substance! If this is the right attitude to take, scientists feeling distaste for dark matter a. | ||
| 506 | |3 Use copy |f Restrictions unspecified |2 star |5 MiAaHDL | ||
| 533 | |a Electronic reproduction. |b [Place of publication not identified] : |c HathiTrust Digital Library, |d 2012. |5 MiAaHDL | ||
| 538 | |a Master and use copy. Digital master created according to Benchmark for Faithful Digital Reproductions of Monographs and Serials, Version 1. Digital Library Federation, December 2002. |u http://purl.oclc.org/DLF/benchrepro0212 |5 MiAaHDL | ||
| 583 | 1 | |a digitized |c 2012 |h HathiTrust Digital Library |l committed to preserve |2 pda |5 MiAaHDL | |
| 650 | 0 | |a Dark matter (Astronomy) |v Congresses. | |
| 650 | 0 | |a Cosmology |v Congresses. | |
| 650 | 0 | |a Galaxies |x Evolution |v Congresses. | |
| 650 | 0 | |a Red shift |v Congresses. | |
| 650 | 0 | |a Large scale structure (Astronomy) |v Congresses. | |
| 650 | 6 | |a Matière sombre (Astronomie) |v Congrès. | |
| 650 | 6 | |a Cosmologie |v Congrès. | |
| 650 | 6 | |a Galaxies |x Évolution |v Congrès. | |
| 650 | 6 | |a Décalage vers le rouge |v Congrès. | |
| 650 | 6 | |a Structure à grande échelle (Astronomie) |v Congrès. | |
| 650 | 7 | |a SCIENCE |x Astronomy. |2 bisacsh | |
| 650 | 7 | |a Red shift |2 fast | |
| 650 | 7 | |a Large scale structure (Astronomy) |2 fast | |
| 650 | 7 | |a Galaxies |x Evolution |2 fast | |
| 650 | 7 | |a Cosmology |2 fast | |
| 650 | 7 | |a Dark matter (Astronomy) |2 fast | |
| 650 | 7 | |a Matière sombre. |2 ram | |
| 655 | 7 | |a Conference papers and proceedings |2 fast | |
| 700 | 1 | |a Bonometto, S. |q (Silvio) |1 https://id.oclc.org/worldcat/entity/E39PCjthDB83qJHQvW4M8Vvd73 |0 http://id.loc.gov/authorities/names/no97023921 | |
| 700 | 1 | |a Primack, J. R. |q (Joel R.) |1 https://id.oclc.org/worldcat/entity/E39PBJc3JWdMCTgqkjh66cHXBP |0 http://id.loc.gov/authorities/names/no97023931 | |
| 700 | 1 | |a Provenzale, A. |q (Antonello) |1 https://id.oclc.org/worldcat/entity/E39PBJjmPDGgX7xF4R3M6bpHG3 |0 http://id.loc.gov/authorities/names/no97023923 | |
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| author_corporate | International School of Physics "Enrico Fermi" Varenna, Italy Società italiana di fisica |
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| author_facet | Bonometto, S. (Silvio) Primack, J. R. (Joel R.) Provenzale, A. (Antonello) International School of Physics "Enrico Fermi" Varenna, Italy Società italiana di fisica |
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| contents | Title Page; Indice; Introductory note; Gruppo fotografico dei partecipanti al Corso fuori testo; Status of cosmological parameters: Omega_0 approx 0.3 vs. Omega = 1; Introduction; Models with mostly cold dark matter; Age of the Universe t_0; Hubble parameter H_0; A) Relative-distance methods; B) Fundamental-physical approaches; Correcting for Virgocentric infall; Cosmological constant Lambda, and t_0 again; Measuring Omega_0; Very-large-scale measurements; Large-scale measurements; Measurements on scales of a few Mpc; Estimates on galaxy halo scales; Clusters. Cluster baryons vs. big-bang nucleosynthesisCluster morphology; Cluster evolution; Early structure formation; Neutrino mass; Conclusions; OBSERVATIONAL DATA; Galaxy redshift surveys; Introduction; Redshift surveys; The Las Campanas Redshift Survey; The beginning of the end?; Beyond the LCRS; Peculiar motions and the Tully-Fisher relation; Introduction; Newtonian theory of small perturbations; The case for large-scale motions; The CMB dipole; Motions at the Local Supercluster scale; The Great Attractor; Bulk flows; The Tully-Fisher relation; Scaling laws; Extinction and the TF relation. Optical and radio velocity widthsThe scatter in the TF relation; Importance of the TF template relation; Results for a cluster sample; An all-sky field spiral sample; Galaxy redshift surveys: caveat emptor; Introduction; Catalogs: tricks and pitfalls; Nearby-galaxy catalogs; Optical catalog; IRAS galaxy surveys; The density field based on redshift catalogs; Morphological and luminosity segregation; The Pisces-Perseus Supercluster; Not a random volume; Measures of clustering; Morphological segregation; Substructure in clusters: Abell 2634; Hidden galaxies; Conclusion. CMBR observations: spectrumIntroduction; Spectrum observations prior to COBE; COBE mission; DIRBE measurements; FIRAS measurements; Comparison of FIRAS with other data; Possible distortions; Summary; CMBR observations: anisotropy; Introduction; History; The COBE DMR; DMR data analysis. Sparse matrix; Correlated noise in the DMR maps; Scaling to large maps; DMR results; Galactic interference; Power spectrum; Comparison to large-scale structure; Future CMB work; Galaxy number counts; Introduction; Modelling the number counts; Luminosity evolution models. The redshift distributions of faint field galaxiesCould we fit the counts in a q_0 = 0.5 Universe model?; Conclusion; Cosmological adventures in the Lyman forest; Introduction; A Lyman-alpha database; The b-N_(HI) distributions: the temperature of the Lyman-alpha clouds; The HI column density distribution; The redshift distribution; The measure of the ultraviolet background from the proximity effect; Clustering properties of the Lyman-alpha clouds; Simulations; ADVANCED STATISTICAL ESTIMATORS; Cosmic velocity fields; Introduction; Gravitational instability; Measuring peculiar velocities. |
| ctrlnum | (OCoLC)812203772 |
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| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.1/126 |
| dewey-search | 523.1/126 |
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| discipline | Physik |
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| genre | Conference papers and proceedings fast |
| genre_facet | Conference papers and proceedings |
| id | ZDB-4-EBA-ocn812203772 |
| illustrated | Illustrated |
| indexdate | 2024-11-27T13:24:59Z |
| institution | BVB |
| institution_GND | http://id.loc.gov/authorities/names/n79145388 |
| isbn | 9781614992172 1614992177 |
| issn | 0074-748X ; |
| language | English |
| oclc_num | 812203772 |
| open_access_boolean | |
| owner | MAIN DE-863 DE-BY-FWS |
| owner_facet | MAIN DE-863 DE-BY-FWS |
| physical | 1 online resource (xviii, 711 pages) : illustrations |
| psigel | ZDB-4-EBA |
| publishDate | 1996 |
| publishDateSearch | 1996 |
| publishDateSort | 1996 |
| publisher | IOS Press, |
| record_format | marc |
| series2 | Proceedings of the International School of Physics "Enrico Fermi", |
| spelling | International School of Physics "Enrico Fermi" (1995 July 25-Aug. 4 : Varenna, Italy) Dark matter in the universe : Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / edited by S. Bonometto, J.R. Primack, and A. Provenzale. Materia oscura nell'universo Amsterdam ; Washington, DC : IOS Press, 1996. 1 online resource (xviii, 711 pages) : illustrations text txt rdacontent computer c rdamedia online resource cr rdacarrier Proceedings of the International School of Physics "Enrico Fermi", 0074-748X ; course 132 Includes bibliographical references. Print version record. Title Page; Indice; Introductory note; Gruppo fotografico dei partecipanti al Corso fuori testo; Status of cosmological parameters: Omega_0 approx 0.3 vs. Omega = 1; Introduction; Models with mostly cold dark matter; Age of the Universe t_0; Hubble parameter H_0; A) Relative-distance methods; B) Fundamental-physical approaches; Correcting for Virgocentric infall; Cosmological constant Lambda, and t_0 again; Measuring Omega_0; Very-large-scale measurements; Large-scale measurements; Measurements on scales of a few Mpc; Estimates on galaxy halo scales; Clusters. Cluster baryons vs. big-bang nucleosynthesisCluster morphology; Cluster evolution; Early structure formation; Neutrino mass; Conclusions; OBSERVATIONAL DATA; Galaxy redshift surveys; Introduction; Redshift surveys; The Las Campanas Redshift Survey; The beginning of the end?; Beyond the LCRS; Peculiar motions and the Tully-Fisher relation; Introduction; Newtonian theory of small perturbations; The case for large-scale motions; The CMB dipole; Motions at the Local Supercluster scale; The Great Attractor; Bulk flows; The Tully-Fisher relation; Scaling laws; Extinction and the TF relation. Optical and radio velocity widthsThe scatter in the TF relation; Importance of the TF template relation; Results for a cluster sample; An all-sky field spiral sample; Galaxy redshift surveys: caveat emptor; Introduction; Catalogs: tricks and pitfalls; Nearby-galaxy catalogs; Optical catalog; IRAS galaxy surveys; The density field based on redshift catalogs; Morphological and luminosity segregation; The Pisces-Perseus Supercluster; Not a random volume; Measures of clustering; Morphological segregation; Substructure in clusters: Abell 2634; Hidden galaxies; Conclusion. CMBR observations: spectrumIntroduction; Spectrum observations prior to COBE; COBE mission; DIRBE measurements; FIRAS measurements; Comparison of FIRAS with other data; Possible distortions; Summary; CMBR observations: anisotropy; Introduction; History; The COBE DMR; DMR data analysis. Sparse matrix; Correlated noise in the DMR maps; Scaling to large maps; DMR results; Galactic interference; Power spectrum; Comparison to large-scale structure; Future CMB work; Galaxy number counts; Introduction; Modelling the number counts; Luminosity evolution models. The redshift distributions of faint field galaxiesCould we fit the counts in a q_0 = 0.5 Universe model?; Conclusion; Cosmological adventures in the Lyman forest; Introduction; A Lyman-alpha database; The b-N_(HI) distributions: the temperature of the Lyman-alpha clouds; The HI column density distribution; The redshift distribution; The measure of the ultraviolet background from the proximity effect; Clustering properties of the Lyman-alpha clouds; Simulations; ADVANCED STATISTICAL ESTIMATORS; Cosmic velocity fields; Introduction; Gravitational instability; Measuring peculiar velocities. Physics and astrophysics came to dark matter through many different routes, finally accepting it, but often with some distaste. It has been noticed that the existence of dark matter is yet another displacement of humans from the centre of the Universe: not only do our planet and our sun have no central position in the Universe, not only are humans just animals (although with a 'specialized' central nervous system), but even the material of which we are made is only a marginal component of the cosmic substance! If this is the right attitude to take, scientists feeling distaste for dark matter a. Use copy Restrictions unspecified star MiAaHDL Electronic reproduction. [Place of publication not identified] : HathiTrust Digital Library, 2012. MiAaHDL Master and use copy. Digital master created according to Benchmark for Faithful Digital Reproductions of Monographs and Serials, Version 1. Digital Library Federation, December 2002. http://purl.oclc.org/DLF/benchrepro0212 MiAaHDL digitized 2012 HathiTrust Digital Library committed to preserve pda MiAaHDL Dark matter (Astronomy) Congresses. Cosmology Congresses. Galaxies Evolution Congresses. Red shift Congresses. Large scale structure (Astronomy) Congresses. Matière sombre (Astronomie) Congrès. Cosmologie Congrès. Galaxies Évolution Congrès. Décalage vers le rouge Congrès. Structure à grande échelle (Astronomie) Congrès. SCIENCE Astronomy. bisacsh Red shift fast Large scale structure (Astronomy) fast Galaxies Evolution fast Cosmology fast Dark matter (Astronomy) fast Matière sombre. ram Conference papers and proceedings fast Bonometto, S. (Silvio) https://id.oclc.org/worldcat/entity/E39PCjthDB83qJHQvW4M8Vvd73 http://id.loc.gov/authorities/names/no97023921 Primack, J. R. (Joel R.) https://id.oclc.org/worldcat/entity/E39PBJc3JWdMCTgqkjh66cHXBP http://id.loc.gov/authorities/names/no97023931 Provenzale, A. (Antonello) https://id.oclc.org/worldcat/entity/E39PBJjmPDGgX7xF4R3M6bpHG3 http://id.loc.gov/authorities/names/no97023923 Società italiana di fisica. http://id.loc.gov/authorities/names/n79145388 Print version: (DLC) 96078118 (OCoLC)36751717 International School of Physics "Enrico Fermi." Proceedings of the International School of Physics "Enrico Fermi" ; course 132. http://id.loc.gov/authorities/names/n42019799 FWS01 ZDB-4-EBA FWS_PDA_EBA https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=651784 Volltext |
| spellingShingle | Dark matter in the universe : Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / Title Page; Indice; Introductory note; Gruppo fotografico dei partecipanti al Corso fuori testo; Status of cosmological parameters: Omega_0 approx 0.3 vs. Omega = 1; Introduction; Models with mostly cold dark matter; Age of the Universe t_0; Hubble parameter H_0; A) Relative-distance methods; B) Fundamental-physical approaches; Correcting for Virgocentric infall; Cosmological constant Lambda, and t_0 again; Measuring Omega_0; Very-large-scale measurements; Large-scale measurements; Measurements on scales of a few Mpc; Estimates on galaxy halo scales; Clusters. Cluster baryons vs. big-bang nucleosynthesisCluster morphology; Cluster evolution; Early structure formation; Neutrino mass; Conclusions; OBSERVATIONAL DATA; Galaxy redshift surveys; Introduction; Redshift surveys; The Las Campanas Redshift Survey; The beginning of the end?; Beyond the LCRS; Peculiar motions and the Tully-Fisher relation; Introduction; Newtonian theory of small perturbations; The case for large-scale motions; The CMB dipole; Motions at the Local Supercluster scale; The Great Attractor; Bulk flows; The Tully-Fisher relation; Scaling laws; Extinction and the TF relation. Optical and radio velocity widthsThe scatter in the TF relation; Importance of the TF template relation; Results for a cluster sample; An all-sky field spiral sample; Galaxy redshift surveys: caveat emptor; Introduction; Catalogs: tricks and pitfalls; Nearby-galaxy catalogs; Optical catalog; IRAS galaxy surveys; The density field based on redshift catalogs; Morphological and luminosity segregation; The Pisces-Perseus Supercluster; Not a random volume; Measures of clustering; Morphological segregation; Substructure in clusters: Abell 2634; Hidden galaxies; Conclusion. CMBR observations: spectrumIntroduction; Spectrum observations prior to COBE; COBE mission; DIRBE measurements; FIRAS measurements; Comparison of FIRAS with other data; Possible distortions; Summary; CMBR observations: anisotropy; Introduction; History; The COBE DMR; DMR data analysis. Sparse matrix; Correlated noise in the DMR maps; Scaling to large maps; DMR results; Galactic interference; Power spectrum; Comparison to large-scale structure; Future CMB work; Galaxy number counts; Introduction; Modelling the number counts; Luminosity evolution models. The redshift distributions of faint field galaxiesCould we fit the counts in a q_0 = 0.5 Universe model?; Conclusion; Cosmological adventures in the Lyman forest; Introduction; A Lyman-alpha database; The b-N_(HI) distributions: the temperature of the Lyman-alpha clouds; The HI column density distribution; The redshift distribution; The measure of the ultraviolet background from the proximity effect; Clustering properties of the Lyman-alpha clouds; Simulations; ADVANCED STATISTICAL ESTIMATORS; Cosmic velocity fields; Introduction; Gravitational instability; Measuring peculiar velocities. Dark matter (Astronomy) Congresses. Cosmology Congresses. Galaxies Evolution Congresses. Red shift Congresses. Large scale structure (Astronomy) Congresses. Matière sombre (Astronomie) Congrès. Cosmologie Congrès. Galaxies Évolution Congrès. Décalage vers le rouge Congrès. Structure à grande échelle (Astronomie) Congrès. SCIENCE Astronomy. bisacsh Red shift fast Large scale structure (Astronomy) fast Galaxies Evolution fast Cosmology fast Dark matter (Astronomy) fast Matière sombre. ram |
| title | Dark matter in the universe : Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / |
| title_alt | Materia oscura nell'universo |
| title_auth | Dark matter in the universe : Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / |
| title_exact_search | Dark matter in the universe : Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / |
| title_full | Dark matter in the universe : Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / edited by S. Bonometto, J.R. Primack, and A. Provenzale. |
| title_fullStr | Dark matter in the universe : Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / edited by S. Bonometto, J.R. Primack, and A. Provenzale. |
| title_full_unstemmed | Dark matter in the universe : Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / edited by S. Bonometto, J.R. Primack, and A. Provenzale. |
| title_short | Dark matter in the universe : |
| title_sort | dark matter in the universe varenna on lake como villa monastero 25 july 4 august 1995 |
| title_sub | Varenna on Lake Como, Villa Monastero, 25 July-4 August 1995 / |
| topic | Dark matter (Astronomy) Congresses. Cosmology Congresses. Galaxies Evolution Congresses. Red shift Congresses. Large scale structure (Astronomy) Congresses. Matière sombre (Astronomie) Congrès. Cosmologie Congrès. Galaxies Évolution Congrès. Décalage vers le rouge Congrès. Structure à grande échelle (Astronomie) Congrès. SCIENCE Astronomy. bisacsh Red shift fast Large scale structure (Astronomy) fast Galaxies Evolution fast Cosmology fast Dark matter (Astronomy) fast Matière sombre. ram |
| topic_facet | Dark matter (Astronomy) Congresses. Cosmology Congresses. Galaxies Evolution Congresses. Red shift Congresses. Large scale structure (Astronomy) Congresses. Matière sombre (Astronomie) Congrès. Cosmologie Congrès. Galaxies Évolution Congrès. Décalage vers le rouge Congrès. Structure à grande échelle (Astronomie) Congrès. SCIENCE Astronomy. Red shift Large scale structure (Astronomy) Galaxies Evolution Cosmology Dark matter (Astronomy) Matière sombre. Conference papers and proceedings |
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