The generalized canonical form of Hori's method for non-canonical systems
Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonica...
Ausführliche Beschreibung
Autor*in: |
---|
Format: |
E-Artikel |
---|---|
Sprache: |
Englisch |
Erschienen: |
1989 |
---|
Umfang: |
9 |
---|
Reproduktion: |
Springer Online Journal Archives 1860-2002 |
---|---|
Übergeordnetes Werk: |
in: Celestial mechanics and dynamical astronomy - 1969, 46(1989) vom: Jan., Seite 49-57 |
Übergeordnetes Werk: |
volume:46 ; year:1989 ; month:01 ; pages:49-57 ; extent:9 |
Links: |
---|
Katalog-ID: |
NLEJ193565668 |
---|
LEADER | 01000caa a22002652 4500 | ||
---|---|---|---|
001 | NLEJ193565668 | ||
003 | DE-627 | ||
005 | 20210707212238.0 | ||
007 | cr uuu---uuuuu | ||
008 | 070526s1989 xx |||||o 00| ||eng c | ||
035 | |a (DE-627)NLEJ193565668 | ||
040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
041 | |a eng | ||
245 | 1 | 0 | |a The generalized canonical form of Hori's method for non-canonical systems |
264 | 1 | |c 1989 | |
300 | |a 9 | ||
336 | |a nicht spezifiziert |b zzz |2 rdacontent | ||
337 | |a nicht spezifiziert |b z |2 rdamedia | ||
338 | |a nicht spezifiziert |b zu |2 rdacarrier | ||
520 | |a Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. | ||
533 | |f Springer Online Journal Archives 1860-2002 | ||
700 | 1 | |a Fernandes, S. S. |4 oth | |
700 | 1 | |a Sessin, W. |4 oth | |
773 | 0 | 8 | |i in |t Celestial mechanics and dynamical astronomy |d 1969 |g 46(1989) vom: Jan., Seite 49-57 |w (DE-627)NLEJ188986588 |w (DE-600)1472552-6 |x 1572-9478 |7 nnns |
773 | 1 | 8 | |g volume:46 |g year:1989 |g month:01 |g pages:49-57 |g extent:9 |
856 | 4 | 0 | |u http://dx.doi.org/10.1007/BF02426712 |
912 | |a GBV_USEFLAG_U | ||
912 | |a ZDB-1-SOJ | ||
912 | |a GBV_NL_ARTICLE | ||
951 | |a AR | ||
952 | |d 46 |j 1989 |c 1 |h 49-57 |g 9 |
matchkey_str |
article:15729478:1989----::hgnrlzdaoiafrohrsehdon |
---|---|
hierarchy_sort_str |
1989 |
publishDate |
1989 |
allfields |
(DE-627)NLEJ193565668 DE-627 ger DE-627 rakwb eng The generalized canonical form of Hori's method for non-canonical systems 1989 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. Springer Online Journal Archives 1860-2002 Fernandes, S. S. oth Sessin, W. oth in Celestial mechanics and dynamical astronomy 1969 46(1989) vom: Jan., Seite 49-57 (DE-627)NLEJ188986588 (DE-600)1472552-6 1572-9478 nnns volume:46 year:1989 month:01 pages:49-57 extent:9 http://dx.doi.org/10.1007/BF02426712 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 46 1989 1 49-57 9 |
spelling |
(DE-627)NLEJ193565668 DE-627 ger DE-627 rakwb eng The generalized canonical form of Hori's method for non-canonical systems 1989 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. Springer Online Journal Archives 1860-2002 Fernandes, S. S. oth Sessin, W. oth in Celestial mechanics and dynamical astronomy 1969 46(1989) vom: Jan., Seite 49-57 (DE-627)NLEJ188986588 (DE-600)1472552-6 1572-9478 nnns volume:46 year:1989 month:01 pages:49-57 extent:9 http://dx.doi.org/10.1007/BF02426712 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 46 1989 1 49-57 9 |
allfields_unstemmed |
(DE-627)NLEJ193565668 DE-627 ger DE-627 rakwb eng The generalized canonical form of Hori's method for non-canonical systems 1989 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. Springer Online Journal Archives 1860-2002 Fernandes, S. S. oth Sessin, W. oth in Celestial mechanics and dynamical astronomy 1969 46(1989) vom: Jan., Seite 49-57 (DE-627)NLEJ188986588 (DE-600)1472552-6 1572-9478 nnns volume:46 year:1989 month:01 pages:49-57 extent:9 http://dx.doi.org/10.1007/BF02426712 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 46 1989 1 49-57 9 |
allfieldsGer |
(DE-627)NLEJ193565668 DE-627 ger DE-627 rakwb eng The generalized canonical form of Hori's method for non-canonical systems 1989 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. Springer Online Journal Archives 1860-2002 Fernandes, S. S. oth Sessin, W. oth in Celestial mechanics and dynamical astronomy 1969 46(1989) vom: Jan., Seite 49-57 (DE-627)NLEJ188986588 (DE-600)1472552-6 1572-9478 nnns volume:46 year:1989 month:01 pages:49-57 extent:9 http://dx.doi.org/10.1007/BF02426712 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 46 1989 1 49-57 9 |
allfieldsSound |
(DE-627)NLEJ193565668 DE-627 ger DE-627 rakwb eng The generalized canonical form of Hori's method for non-canonical systems 1989 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. Springer Online Journal Archives 1860-2002 Fernandes, S. S. oth Sessin, W. oth in Celestial mechanics and dynamical astronomy 1969 46(1989) vom: Jan., Seite 49-57 (DE-627)NLEJ188986588 (DE-600)1472552-6 1572-9478 nnns volume:46 year:1989 month:01 pages:49-57 extent:9 http://dx.doi.org/10.1007/BF02426712 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 46 1989 1 49-57 9 |
language |
English |
source |
in Celestial mechanics and dynamical astronomy 46(1989) vom: Jan., Seite 49-57 volume:46 year:1989 month:01 pages:49-57 extent:9 |
sourceStr |
in Celestial mechanics and dynamical astronomy 46(1989) vom: Jan., Seite 49-57 volume:46 year:1989 month:01 pages:49-57 extent:9 |
format_phy_str_mv |
Article |
institution |
findex.gbv.de |
isfreeaccess_bool |
false |
container_title |
Celestial mechanics and dynamical astronomy |
authorswithroles_txt_mv |
Fernandes, S. S. @@oth@@ Sessin, W. @@oth@@ |
publishDateDaySort_date |
1989-01-01T00:00:00Z |
hierarchy_top_id |
NLEJ188986588 |
id |
NLEJ193565668 |
language_de |
englisch |
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">NLEJ193565668</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210707212238.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070526s1989 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ193565668</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="245" ind1="1" ind2="0"><subfield code="a">The generalized canonical form of Hori's method for non-canonical systems</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1989</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">9</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Springer Online Journal Archives 1860-2002</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fernandes, S. S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sessin, W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Celestial mechanics and dynamical astronomy</subfield><subfield code="d">1969</subfield><subfield code="g">46(1989) vom: Jan., Seite 49-57</subfield><subfield code="w">(DE-627)NLEJ188986588</subfield><subfield code="w">(DE-600)1472552-6</subfield><subfield code="x">1572-9478</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:46</subfield><subfield code="g">year:1989</subfield><subfield code="g">month:01</subfield><subfield code="g">pages:49-57</subfield><subfield code="g">extent:9</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://dx.doi.org/10.1007/BF02426712</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SOJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">46</subfield><subfield code="j">1989</subfield><subfield code="c">1</subfield><subfield code="h">49-57</subfield><subfield code="g">9</subfield></datafield></record></collection>
|
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">NLEJ193565668</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210707212238.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070526s1989 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ193565668</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="245" ind1="1" ind2="0"><subfield code="a">The generalized canonical form of Hori's method for non-canonical systems</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1989</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">9</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Springer Online Journal Archives 1860-2002</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fernandes, S. S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sessin, W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Celestial mechanics and dynamical astronomy</subfield><subfield code="d">1969</subfield><subfield code="g">46(1989) vom: Jan., Seite 49-57</subfield><subfield code="w">(DE-627)NLEJ188986588</subfield><subfield code="w">(DE-600)1472552-6</subfield><subfield code="x">1572-9478</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:46</subfield><subfield code="g">year:1989</subfield><subfield code="g">month:01</subfield><subfield code="g">pages:49-57</subfield><subfield code="g">extent:9</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://dx.doi.org/10.1007/BF02426712</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SOJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">46</subfield><subfield code="j">1989</subfield><subfield code="c">1</subfield><subfield code="h">49-57</subfield><subfield code="g">9</subfield></datafield></record></collection>
|
series2 |
Springer Online Journal Archives 1860-2002 |
ppnlink_with_tag_str_mv |
@@773@@(DE-627)NLEJ188986588 |
format |
electronic Article |
delete_txt_mv |
keep |
collection |
NL |
remote_str |
true |
illustrated |
Not Illustrated |
issn |
1572-9478 |
topic_title |
The generalized canonical form of Hori's method for non-canonical systems |
format_facet |
Elektronische Aufsätze Aufsätze Elektronische Ressource |
format_main_str_mv |
Text Zeitschrift/Artikel |
carriertype_str_mv |
zu |
author2_variant |
s s f ss ssf w s ws |
hierarchy_parent_title |
Celestial mechanics and dynamical astronomy |
hierarchy_parent_id |
NLEJ188986588 |
hierarchy_top_title |
Celestial mechanics and dynamical astronomy |
isfreeaccess_txt |
false |
familylinks_str_mv |
(DE-627)NLEJ188986588 (DE-600)1472552-6 |
title |
The generalized canonical form of Hori's method for non-canonical systems |
spellingShingle |
The generalized canonical form of Hori's method for non-canonical systems |
ctrlnum |
(DE-627)NLEJ193565668 |
title_full |
The generalized canonical form of Hori's method for non-canonical systems |
journal |
Celestial mechanics and dynamical astronomy |
journalStr |
Celestial mechanics and dynamical astronomy |
lang_code |
eng |
isOA_bool |
false |
recordtype |
marc |
publishDateSort |
1989 |
contenttype_str_mv |
zzz |
container_start_page |
49 |
container_volume |
46 |
physical |
9 |
format_se |
Elektronische Aufsätze |
title_sort |
the generalized canonical form of hori's method for non-canonical systems |
title_auth |
The generalized canonical form of Hori's method for non-canonical systems |
abstract |
Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. |
abstractGer |
Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. |
abstract_unstemmed |
Abstract Any dynamical system can be put in generalized canonical form through the introduction of a set of auxiliary ‘conjugate’ variables or momenta and solved by perturbation theory based on Lie series. The application of Hori's method for generalized canonical system leads to a new canonical transformation — the Mathieu transformation — defined by the solution of the Hori auxiliary system. This new transformation simplifies the algorithm since the inversion of the solution of the Hori auxiliary system is no longer necessary. In this paper, we wish to show some peculiarities of this technique. |
collection_details |
GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE |
title_short |
The generalized canonical form of Hori's method for non-canonical systems |
url |
http://dx.doi.org/10.1007/BF02426712 |
remote_bool |
true |
author2 |
Fernandes, S. S. Sessin, W. |
author2Str |
Fernandes, S. S. Sessin, W. |
ppnlink |
NLEJ188986588 |
mediatype_str_mv |
z |
isOA_txt |
false |
hochschulschrift_bool |
false |
author2_role |
oth oth |
up_date |
2024-07-05T22:04:38.272Z |
_version_ |
1803778343066140672 |
score |
7.4012003 |