Soliton solutions and their stability for the flow of relativistic fluids through channels
Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solut...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Lerche, I. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1980 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© D. Reidel Publishing Co 1980 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 68(1980), 1 vom: März, Seite 207-219 |
|---|---|
| Übergeordnetes Werk: |
volume:68 ; year:1980 ; number:1 ; month:03 ; pages:207-219 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00641656 |
|---|
| Katalog-ID: |
OLC2066137979 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2066137979 | ||
| 003 | DE-627 | ||
| 005 | 20230502211549.0 | ||
| 007 | tu | ||
| 008 | 200820s1980 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1007/BF00641656 |2 doi | |
| 035 | |a (DE-627)OLC2066137979 | ||
| 035 | |a (DE-He213)BF00641656-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 Lerche, I. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Soliton solutions and their stability for the flow of relativistic fluids through channels |
| 264 | 1 | |c 1980 | |
| 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 Co 1980 | ||
| 520 | |a Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. | ||
| 650 | 4 | |a Soliton | |
| 650 | 4 | |a Soliton Solution | |
| 650 | 4 | |a Radio Galaxy | |
| 650 | 4 | |a Relativistic Fluid | |
| 650 | 4 | |a Soliton Mode | |
| 700 | 1 | |a Wiita, P. J. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Astrophysics and space science |d Kluwer Academic Publishers, 1968 |g 68(1980), 1 vom: März, Seite 207-219 |w (DE-627)129062723 |w (DE-600)629-4 |w (DE-576)014393522 |x 0004-640X |7 nnns |
| 773 | 1 | 8 | |g volume:68 |g year:1980 |g number:1 |g month:03 |g pages:207-219 |
| 856 | 4 | 1 | |u https://doi.org/10.1007/BF00641656 |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_20 | ||
| 912 | |a GBV_ILN_21 | ||
| 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_4035 | ||
| 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 68 |j 1980 |e 1 |c 03 |h 207-219 | ||
| author_variant |
i l il p j w pj pjw |
|---|---|
| matchkey_str |
article:0004640X:1980----::oiosltosntertbltfrhfoorltvsi |
| hierarchy_sort_str |
1980 |
| publishDate |
1980 |
| allfields |
10.1007/BF00641656 doi (DE-627)OLC2066137979 (DE-He213)BF00641656-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lerche, I. verfasserin aut Soliton solutions and their stability for the flow of relativistic fluids through channels 1980 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1980 Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. Soliton Soliton Solution Radio Galaxy Relativistic Fluid Soliton Mode Wiita, P. J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 68(1980), 1 vom: März, Seite 207-219 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:68 year:1980 number:1 month:03 pages:207-219 https://doi.org/10.1007/BF00641656 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 68 1980 1 03 207-219 |
| spelling |
10.1007/BF00641656 doi (DE-627)OLC2066137979 (DE-He213)BF00641656-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lerche, I. verfasserin aut Soliton solutions and their stability for the flow of relativistic fluids through channels 1980 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1980 Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. Soliton Soliton Solution Radio Galaxy Relativistic Fluid Soliton Mode Wiita, P. J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 68(1980), 1 vom: März, Seite 207-219 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:68 year:1980 number:1 month:03 pages:207-219 https://doi.org/10.1007/BF00641656 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 68 1980 1 03 207-219 |
| allfields_unstemmed |
10.1007/BF00641656 doi (DE-627)OLC2066137979 (DE-He213)BF00641656-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lerche, I. verfasserin aut Soliton solutions and their stability for the flow of relativistic fluids through channels 1980 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1980 Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. Soliton Soliton Solution Radio Galaxy Relativistic Fluid Soliton Mode Wiita, P. J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 68(1980), 1 vom: März, Seite 207-219 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:68 year:1980 number:1 month:03 pages:207-219 https://doi.org/10.1007/BF00641656 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 68 1980 1 03 207-219 |
| allfieldsGer |
10.1007/BF00641656 doi (DE-627)OLC2066137979 (DE-He213)BF00641656-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lerche, I. verfasserin aut Soliton solutions and their stability for the flow of relativistic fluids through channels 1980 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1980 Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. Soliton Soliton Solution Radio Galaxy Relativistic Fluid Soliton Mode Wiita, P. J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 68(1980), 1 vom: März, Seite 207-219 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:68 year:1980 number:1 month:03 pages:207-219 https://doi.org/10.1007/BF00641656 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 68 1980 1 03 207-219 |
| allfieldsSound |
10.1007/BF00641656 doi (DE-627)OLC2066137979 (DE-He213)BF00641656-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Lerche, I. verfasserin aut Soliton solutions and their stability for the flow of relativistic fluids through channels 1980 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1980 Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. Soliton Soliton Solution Radio Galaxy Relativistic Fluid Soliton Mode Wiita, P. J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 68(1980), 1 vom: März, Seite 207-219 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:68 year:1980 number:1 month:03 pages:207-219 https://doi.org/10.1007/BF00641656 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 68 1980 1 03 207-219 |
| language |
English |
| source |
Enthalten in Astrophysics and space science 68(1980), 1 vom: März, Seite 207-219 volume:68 year:1980 number:1 month:03 pages:207-219 |
| sourceStr |
Enthalten in Astrophysics and space science 68(1980), 1 vom: März, Seite 207-219 volume:68 year:1980 number:1 month:03 pages:207-219 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Soliton Soliton Solution Radio Galaxy Relativistic Fluid Soliton Mode |
| dewey-raw |
520 |
| isfreeaccess_bool |
false |
| container_title |
Astrophysics and space science |
| authorswithroles_txt_mv |
Lerche, I. @@aut@@ Wiita, P. J. @@aut@@ |
| publishDateDaySort_date |
1980-03-01T00:00:00Z |
| hierarchy_top_id |
129062723 |
| dewey-sort |
3520 |
| id |
OLC2066137979 |
| 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">OLC2066137979</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502211549.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1980 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF00641656</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066137979</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF00641656-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">Lerche, I.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Soliton solutions and their stability for the flow of relativistic fluids through channels</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1980</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 Co 1980</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Soliton</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Soliton Solution</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radio Galaxy</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Relativistic Fluid</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Soliton Mode</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wiita, P. J.</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">68(1980), 1 vom: März, Seite 207-219</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:68</subfield><subfield code="g">year:1980</subfield><subfield code="g">number:1</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:207-219</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00641656</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_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_21</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_4035</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">68</subfield><subfield code="j">1980</subfield><subfield code="e">1</subfield><subfield code="c">03</subfield><subfield code="h">207-219</subfield></datafield></record></collection>
|
| author |
Lerche, I. |
| spellingShingle |
Lerche, I. ddc 520 ssgn 16,12 misc Soliton misc Soliton Solution misc Radio Galaxy misc Relativistic Fluid misc Soliton Mode Soliton solutions and their stability for the flow of relativistic fluids through channels |
| authorStr |
Lerche, I. |
| 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 Soliton solutions and their stability for the flow of relativistic fluids through channels Soliton Soliton Solution Radio Galaxy Relativistic Fluid Soliton Mode |
| topic |
ddc 520 ssgn 16,12 misc Soliton misc Soliton Solution misc Radio Galaxy misc Relativistic Fluid misc Soliton Mode |
| topic_unstemmed |
ddc 520 ssgn 16,12 misc Soliton misc Soliton Solution misc Radio Galaxy misc Relativistic Fluid misc Soliton Mode |
| topic_browse |
ddc 520 ssgn 16,12 misc Soliton misc Soliton Solution misc Radio Galaxy misc Relativistic Fluid misc Soliton Mode |
| 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 |
Soliton solutions and their stability for the flow of relativistic fluids through channels |
| ctrlnum |
(DE-627)OLC2066137979 (DE-He213)BF00641656-p |
| title_full |
Soliton solutions and their stability for the flow of relativistic fluids through channels |
| author_sort |
Lerche, I. |
| 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 |
1980 |
| contenttype_str_mv |
txt |
| container_start_page |
207 |
| author_browse |
Lerche, I. Wiita, P. J. |
| container_volume |
68 |
| class |
520 530 620 VZ 16,12 ssgn |
| format_se |
Aufsätze |
| author-letter |
Lerche, I. |
| doi_str_mv |
10.1007/BF00641656 |
| dewey-full |
520 530 620 |
| title_sort |
soliton solutions and their stability for the flow of relativistic fluids through channels |
| title_auth |
Soliton solutions and their stability for the flow of relativistic fluids through channels |
| abstract |
Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. © D. Reidel Publishing Co 1980 |
| abstractGer |
Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. © D. Reidel Publishing Co 1980 |
| abstract_unstemmed |
Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay. © D. Reidel Publishing Co 1980 |
| 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 |
| container_issue |
1 |
| title_short |
Soliton solutions and their stability for the flow of relativistic fluids through channels |
| url |
https://doi.org/10.1007/BF00641656 |
| remote_bool |
false |
| author2 |
Wiita, P. J. |
| author2Str |
Wiita, P. J. |
| ppnlink |
129062723 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1007/BF00641656 |
| up_date |
2024-07-04T03:50:49.918Z |
| _version_ |
1803618929792253952 |
| 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">OLC2066137979</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502211549.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1980 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF00641656</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066137979</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF00641656-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">Lerche, I.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Soliton solutions and their stability for the flow of relativistic fluids through channels</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1980</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 Co 1980</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract We analyze the flow of a perfect relativistic fluid in a confining channel of variable cross-section — a situation that is relevant for models of radio galaxies. Families of soliton-like solutions are found and their topologies described. However, a perturbative investigation of these solutions indicates that all such soliton modes are unstable, and would eventually decay.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Soliton</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Soliton Solution</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radio Galaxy</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Relativistic Fluid</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Soliton Mode</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wiita, P. J.</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">68(1980), 1 vom: März, Seite 207-219</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:68</subfield><subfield code="g">year:1980</subfield><subfield code="g">number:1</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:207-219</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00641656</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_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_21</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_4035</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">68</subfield><subfield code="j">1980</subfield><subfield code="e">1</subfield><subfield code="c">03</subfield><subfield code="h">207-219</subfield></datafield></record></collection>
|
| score |
7.4016542 |