Large-scale inhomogeneities and the cosmological principle
Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity fiel...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Lukaćs, B. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1985 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© D. Reidel Publishing Company 1985 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 114(1985), 2 vom: Sept., Seite 211-231 |
|---|---|
| Übergeordnetes Werk: |
volume:114 ; year:1985 ; number:2 ; month:09 ; pages:211-231 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00653966 |
|---|
| Katalog-ID: |
OLC2066157597 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2066157597 | ||
| 003 | DE-627 | ||
| 005 | 20230502211931.0 | ||
| 007 | tu | ||
| 008 | 200820s1985 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1007/BF00653966 |2 doi | |
| 035 | |a (DE-627)OLC2066157597 | ||
| 035 | |a (DE-He213)BF00653966-p | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 520 |a 530 |a 620 |q VZ |
| 084 | |a 16,12 |2 ssgn | ||
| 100 | 1 | |a Lukaćs, B. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Large-scale inhomogeneities and the cosmological principle |
| 264 | 1 | |c 1985 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
| 338 | |a Band |b nc |2 rdacarrier | ||
| 500 | |a © D. Reidel Publishing Company 1985 | ||
| 520 | |a Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. | ||
| 650 | 4 | |a Velocity Field | |
| 650 | 4 | |a Conformal Symmetry | |
| 650 | 4 | |a Symmetry Principle | |
| 650 | 4 | |a Cosmologic Principle | |
| 650 | 4 | |a Strong Symmetry | |
| 700 | 1 | |a Mészáros, A. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Astrophysics and space science |d Kluwer Academic Publishers, 1968 |g 114(1985), 2 vom: Sept., Seite 211-231 |w (DE-627)129062723 |w (DE-600)629-4 |w (DE-576)014393522 |x 0004-640X |7 nnns |
| 773 | 1 | 8 | |g volume:114 |g year:1985 |g number:2 |g month:09 |g pages:211-231 |
| 856 | 4 | 1 | |u https://doi.org/10.1007/BF00653966 |z lizenzpflichtig |3 Volltext |
| 912 | |a GBV_USEFLAG_A | ||
| 912 | |a SYSFLAG_A | ||
| 912 | |a GBV_OLC | ||
| 912 | |a SSG-OLC-TEC | ||
| 912 | |a SSG-OLC-PHY | ||
| 912 | |a SSG-OLC-AST | ||
| 912 | |a SSG-OPC-AST | ||
| 912 | |a GBV_ILN_11 | ||
| 912 | |a GBV_ILN_22 | ||
| 912 | |a GBV_ILN_24 | ||
| 912 | |a GBV_ILN_31 | ||
| 912 | |a GBV_ILN_40 | ||
| 912 | |a GBV_ILN_47 | ||
| 912 | |a GBV_ILN_70 | ||
| 912 | |a GBV_ILN_2002 | ||
| 912 | |a GBV_ILN_2279 | ||
| 912 | |a GBV_ILN_2286 | ||
| 912 | |a GBV_ILN_4012 | ||
| 912 | |a GBV_ILN_4046 | ||
| 912 | |a GBV_ILN_4082 | ||
| 912 | |a GBV_ILN_4103 | ||
| 912 | |a GBV_ILN_4305 | ||
| 912 | |a GBV_ILN_4306 | ||
| 912 | |a GBV_ILN_4700 | ||
| 951 | |a AR | ||
| 952 | |d 114 |j 1985 |e 2 |c 09 |h 211-231 | ||
| author_variant |
b l bl a m am |
|---|---|
| matchkey_str |
article:0004640X:1985----::agsaenooeeteadhcsoo |
| hierarchy_sort_str |
1985 |
| publishDate |
1985 |
| allfields |
10.1007/BF00653966 doi (DE-627)OLC2066157597 (DE-He213)BF00653966-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lukaćs, B. verfasserin aut Large-scale inhomogeneities and the cosmological principle 1985 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1985 Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. Velocity Field Conformal Symmetry Symmetry Principle Cosmologic Principle Strong Symmetry Mészáros, A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 114(1985), 2 vom: Sept., Seite 211-231 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:114 year:1985 number:2 month:09 pages:211-231 https://doi.org/10.1007/BF00653966 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 114 1985 2 09 211-231 |
| spelling |
10.1007/BF00653966 doi (DE-627)OLC2066157597 (DE-He213)BF00653966-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lukaćs, B. verfasserin aut Large-scale inhomogeneities and the cosmological principle 1985 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1985 Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. Velocity Field Conformal Symmetry Symmetry Principle Cosmologic Principle Strong Symmetry Mészáros, A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 114(1985), 2 vom: Sept., Seite 211-231 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:114 year:1985 number:2 month:09 pages:211-231 https://doi.org/10.1007/BF00653966 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 114 1985 2 09 211-231 |
| allfields_unstemmed |
10.1007/BF00653966 doi (DE-627)OLC2066157597 (DE-He213)BF00653966-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lukaćs, B. verfasserin aut Large-scale inhomogeneities and the cosmological principle 1985 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1985 Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. Velocity Field Conformal Symmetry Symmetry Principle Cosmologic Principle Strong Symmetry Mészáros, A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 114(1985), 2 vom: Sept., Seite 211-231 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:114 year:1985 number:2 month:09 pages:211-231 https://doi.org/10.1007/BF00653966 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 114 1985 2 09 211-231 |
| allfieldsGer |
10.1007/BF00653966 doi (DE-627)OLC2066157597 (DE-He213)BF00653966-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lukaćs, B. verfasserin aut Large-scale inhomogeneities and the cosmological principle 1985 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1985 Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. Velocity Field Conformal Symmetry Symmetry Principle Cosmologic Principle Strong Symmetry Mészáros, A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 114(1985), 2 vom: Sept., Seite 211-231 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:114 year:1985 number:2 month:09 pages:211-231 https://doi.org/10.1007/BF00653966 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 114 1985 2 09 211-231 |
| allfieldsSound |
10.1007/BF00653966 doi (DE-627)OLC2066157597 (DE-He213)BF00653966-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lukaćs, B. verfasserin aut Large-scale inhomogeneities and the cosmological principle 1985 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1985 Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. Velocity Field Conformal Symmetry Symmetry Principle Cosmologic Principle Strong Symmetry Mészáros, A. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 114(1985), 2 vom: Sept., Seite 211-231 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:114 year:1985 number:2 month:09 pages:211-231 https://doi.org/10.1007/BF00653966 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 114 1985 2 09 211-231 |
| language |
English |
| source |
Enthalten in Astrophysics and space science 114(1985), 2 vom: Sept., Seite 211-231 volume:114 year:1985 number:2 month:09 pages:211-231 |
| sourceStr |
Enthalten in Astrophysics and space science 114(1985), 2 vom: Sept., Seite 211-231 volume:114 year:1985 number:2 month:09 pages:211-231 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Velocity Field Conformal Symmetry Symmetry Principle Cosmologic Principle Strong Symmetry |
| dewey-raw |
520 |
| isfreeaccess_bool |
false |
| container_title |
Astrophysics and space science |
| authorswithroles_txt_mv |
Lukaćs, B. @@aut@@ Mészáros, A. @@aut@@ |
| publishDateDaySort_date |
1985-09-01T00:00:00Z |
| hierarchy_top_id |
129062723 |
| dewey-sort |
3520 |
| id |
OLC2066157597 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066157597</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502211931.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1985 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF00653966</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066157597</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF00653966-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Lukaćs, B.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Large-scale inhomogeneities and the cosmological principle</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1985</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© D. Reidel Publishing Company 1985</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Velocity Field</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Conformal Symmetry</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Symmetry Principle</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Cosmologic Principle</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Strong Symmetry</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mészáros, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Kluwer Academic Publishers, 1968</subfield><subfield code="g">114(1985), 2 vom: Sept., Seite 211-231</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:114</subfield><subfield code="g">year:1985</subfield><subfield code="g">number:2</subfield><subfield code="g">month:09</subfield><subfield code="g">pages:211-231</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00653966</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4082</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4103</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4305</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">114</subfield><subfield code="j">1985</subfield><subfield code="e">2</subfield><subfield code="c">09</subfield><subfield code="h">211-231</subfield></datafield></record></collection>
|
| author |
Lukaćs, B. |
| spellingShingle |
Lukaćs, B. ddc 520 ssgn 16,12 misc Velocity Field misc Conformal Symmetry misc Symmetry Principle misc Cosmologic Principle misc Strong Symmetry Large-scale inhomogeneities and the cosmological principle |
| authorStr |
Lukaćs, B. |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)129062723 |
| format |
Article |
| dewey-ones |
520 - Astronomy & allied sciences 530 - Physics 620 - Engineering & allied operations |
| delete_txt_mv |
keep |
| author_role |
aut aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0004-640X |
| topic_title |
520 530 620 VZ 16,12 ssgn Large-scale inhomogeneities and the cosmological principle Velocity Field Conformal Symmetry Symmetry Principle Cosmologic Principle Strong Symmetry |
| topic |
ddc 520 ssgn 16,12 misc Velocity Field misc Conformal Symmetry misc Symmetry Principle misc Cosmologic Principle misc Strong Symmetry |
| topic_unstemmed |
ddc 520 ssgn 16,12 misc Velocity Field misc Conformal Symmetry misc Symmetry Principle misc Cosmologic Principle misc Strong Symmetry |
| topic_browse |
ddc 520 ssgn 16,12 misc Velocity Field misc Conformal Symmetry misc Symmetry Principle misc Cosmologic Principle misc Strong Symmetry |
| format_facet |
Aufsätze Gedruckte Aufsätze |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
nc |
| hierarchy_parent_title |
Astrophysics and space science |
| hierarchy_parent_id |
129062723 |
| dewey-tens |
520 - Astronomy 530 - Physics 620 - Engineering |
| hierarchy_top_title |
Astrophysics and space science |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)129062723 (DE-600)629-4 (DE-576)014393522 |
| title |
Large-scale inhomogeneities and the cosmological principle |
| ctrlnum |
(DE-627)OLC2066157597 (DE-He213)BF00653966-p |
| title_full |
Large-scale inhomogeneities and the cosmological principle |
| author_sort |
Lukaćs, B. |
| journal |
Astrophysics and space science |
| journalStr |
Astrophysics and space science |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science 600 - Technology |
| recordtype |
marc |
| publishDateSort |
1985 |
| contenttype_str_mv |
txt |
| container_start_page |
211 |
| author_browse |
Lukaćs, B. Mészáros, A. |
| container_volume |
114 |
| class |
520 530 620 VZ 16,12 ssgn |
| format_se |
Aufsätze |
| author-letter |
Lukaćs, B. |
| doi_str_mv |
10.1007/BF00653966 |
| dewey-full |
520 530 620 |
| title_sort |
large-scale inhomogeneities and the cosmological principle |
| title_auth |
Large-scale inhomogeneities and the cosmological principle |
| abstract |
Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. © D. Reidel Publishing Company 1985 |
| abstractGer |
Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. © D. Reidel Publishing Company 1985 |
| abstract_unstemmed |
Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered. © D. Reidel Publishing Company 1985 |
| collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 |
| container_issue |
2 |
| title_short |
Large-scale inhomogeneities and the cosmological principle |
| url |
https://doi.org/10.1007/BF00653966 |
| remote_bool |
false |
| author2 |
Mészáros, A. |
| author2Str |
Mészáros, A. |
| ppnlink |
129062723 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1007/BF00653966 |
| up_date |
2024-07-04T03:53:12.531Z |
| _version_ |
1803619079332823040 |
| fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066157597</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502211931.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1985 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF00653966</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066157597</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF00653966-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Lukaćs, B.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Large-scale inhomogeneities and the cosmological principle</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1985</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© D. Reidel Publishing Company 1985</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The compatibility of cosmologic principles and possible large-scale inhomogeneities of the Universe is discussed. It seems that the strongest symmetry principle compatible with reasonable inhomogeneities is full conformal symmetry in the three-space defined by the cosmological velocity field; but even then the standard model is isolated from inhomogeneous ones when the whole evolution is considered.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Velocity Field</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Conformal Symmetry</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Symmetry Principle</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Cosmologic Principle</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Strong Symmetry</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mészáros, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Kluwer Academic Publishers, 1968</subfield><subfield code="g">114(1985), 2 vom: Sept., Seite 211-231</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:114</subfield><subfield code="g">year:1985</subfield><subfield code="g">number:2</subfield><subfield code="g">month:09</subfield><subfield code="g">pages:211-231</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00653966</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4082</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4103</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4305</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">114</subfield><subfield code="j">1985</subfield><subfield code="e">2</subfield><subfield code="c">09</subfield><subfield code="h">211-231</subfield></datafield></record></collection>
|
| score |
7.3990517 |