{"id":{"repo_id":"greece","oai_identifier":"oai:10442/1748"},"canonical_url":"https://search.dev.ndltd.org/etd/greece/oai:10442/1748","repository":{"repo_id":"greece","name":"Greek National Archive of PhD Theses","base_url":"https://phdtheses.ekt.gr/eadd_oai/request"},"display":{"title":"ΣΥΜΒΟΛΗ ΣΤΟ ΠΡΟΒΛΗΜΑ ΤΗΣ ΔΙΑΦΟΡΙΚΗΣ ΠΕΡΙΣΤΡΟΦΗΣ ΕΝΟΣ ΛΕΥΚΟΥ ΝΑΝΟΥ ΜΕ ΑΝΑΠΤΥΞΗ ΚΑΙ ΕΦΑΡΜΟΓΗ ΘΕΩΡΙΩΝ ΔΙΑΤΑΡΑΧΗΣ","abstract":"THIS THESIS REPRESENTS A THEORETICAL STUDY OF AN EITHER UNIFORM OR NONUNIFORM ROTATION OF A COMPLETELY DEGENERATE ELECTRON GAS CONTINUUM, FORMING A WHITE DWAR. THE AIM OF CHAPTER 1 IS TO SPECIFY THE STRUCTURE DIFFERENTIALLY ROTATING WHITE DWARF BY EXTENDING CHANDRASEKHAR'S METHOD TO INCLUDE UP TO THIRD ORDER TERMS IN THE ROTATIONAL PERTURBATION PARAMETER. IN CHAPTERS II AND III WE OBTAIN NUMERICAL RESULTS THAT PERMIT US THE DETERMINATION OF THE WHITE DWARF STRUCTURE FORUNIFORM ROTATION AND FOR A WEAK, MEDIUM, OR EVEN STRONG DIFFERENTIAL ROTATION.THE RESULTS OBTAINED BY A BOTH SIMPLE AND TIME-SAVING TECHNIQUE ARE THEN COMPARED TO THOSE OF PREVIOUS INVESTIGATIONS, AND THEY ARE FOUND TO BE IN AGREEMENT WITH THEM. THE AIM OF CHAPTER IV IS TO DETERMINE THE STRUCTURE OF A DIFFERENTIALLY ROTATING MAGNETIC WHITE DWARF BY EXTENDING CHANDRASEKHAR'S METHOD TO INCLUDE UP TO SECOND ORDER TERMS IN BOTH THE ROTATIONAL AND THE MAGNETIC PERTURBATIONPARAMETERS. IN CHAPTER V, WE OBTAIN NUMERICAL RESULTS THAT PERMIT US THE DETERMINATION OF THE WHITE DWARF STRUCTURE FOR UNIFORM ROTATION AND FOR A WEAK, MEDIUM OR EVEN STRONG DIFFERENTIAL ROTATION, IN THE PRESENCE OF AN EITHER WEAK OR STRONG MAGNETIC FIELD.","abstract_html":"THIS THESIS REPRESENTS A THEORETICAL STUDY OF AN EITHER UNIFORM OR NONUNIFORM ROTATION OF A COMPLETELY DEGENERATE ELECTRON GAS CONTINUUM, FORMING A WHITE DWAR. THE AIM OF CHAPTER 1 IS TO SPECIFY THE STRUCTURE DIFFERENTIALLY ROTATING WHITE DWARF BY EXTENDING CHANDRASEKHAR'S METHOD TO INCLUDE UP TO THIRD ORDER TERMS IN THE ROTATIONAL PERTURBATION PARAMETER. IN CHAPTERS II AND III WE OBTAIN NUMERICAL RESULTS THAT PERMIT US THE DETERMINATION OF THE WHITE DWARF STRUCTURE FORUNIFORM ROTATION AND FOR A WEAK, MEDIUM, OR EVEN STRONG DIFFERENTIAL ROTATION.THE RESULTS OBTAINED BY A BOTH SIMPLE AND TIME-SAVING TECHNIQUE ARE THEN COMPARED TO THOSE OF PREVIOUS INVESTIGATIONS, AND THEY ARE FOUND TO BE IN AGREEMENT WITH THEM. THE AIM OF CHAPTER IV IS TO DETERMINE THE STRUCTURE OF A DIFFERENTIALLY ROTATING MAGNETIC WHITE DWARF BY EXTENDING CHANDRASEKHAR'S METHOD TO INCLUDE UP TO SECOND ORDER TERMS IN BOTH THE ROTATIONAL AND THE MAGNETIC PERTURBATIONPARAMETERS. IN CHAPTER V, WE OBTAIN NUMERICAL RESULTS THAT PERMIT US THE DETERMINATION OF THE WHITE DWARF STRUCTURE FOR UNIFORM ROTATION AND FOR A WEAK, MEDIUM OR EVEN STRONG DIFFERENTIAL ROTATION, IN THE PRESENCE OF AN EITHER WEAK OR STRONG MAGNETIC FIELD.","abstract_has_math":false,"creators":["Hadjopoulos, Anastasios","Χατζόπουλος, Αναστάσιος"],"institution":"University of Patras","degree_name":null,"degree_level":null,"degree_discipline":null,"degree_department":null,"school":null,"contributors":[],"advisors":[],"committee_chairs":[],"committee_members":[],"year":1991,"date_issued":"1991","date_published":"1991","updated_at":"2026-07-24T02:25:05Z","subjects":["Αριθμητικές μέθοδοι","Αριθμητικές τεχνικές","ΑΣΤΕΡΕΣ: ΔΟΜΗ","Αστέρες: Λευκοί Νάνοι","Αστέρες: Μαγνητοϋδροδυναμική","ΑΣΤΕΡΕΣ: ΠΕΡΙΣΤΡΟΦΗ","Υπολογιστική αστροφυσική","Computational astrophysics","Numerical methods","Numerical techniques","Stars: Magnetohydrodynamics","STARS: ROTATION","STARS: STRUCTURE","Stars: White Dwarfs","Φυσικές Επιστήμες","Φυσική","Natural Sciences","Physical Sciences"],"languages":["gre"],"rights":[],"rights_urls":[],"identifier_entries":[{"key":"dc:identifier","label":"Identifier","values":["10.12681/eadd/1748"],"render_values":[{"text":"10.12681/eadd/1748","href":"https://doi.org/10.12681/eadd/1748","code":true}]}]},"links":{"outbound_url":"http://hdl.handle.net/10442/hedi/1748","outbound_label":"Handle","outbound_source":"dc:identifier"},"metadata_groups":[{"id":"people","label":"People","entries":[{"key":"dc:creator","label":"Author","values":["Hadjopoulos, Anastasios","Χατζόπουλος, Αναστάσιος"]}]},{"id":"academic_context","label":"Academic Context","entries":[{"key":"dc:date","label":"Dc Date","values":["1991"]},{"key":"dc:publisher","label":"Institution","values":["University of Patras","Πανεπιστήμιο Πατρών"]},{"key":"dc:type","label":"Dc Type","values":["PhD Thesis"]}]},{"id":"subjects_keywords","label":"Subjects and Keywords","entries":[{"key":"dc:subject","label":"Dc Subject","values":["Αριθμητικές μέθοδοι","Αριθμητικές τεχνικές","ΑΣΤΕΡΕΣ: ΔΟΜΗ","Αστέρες: Λευκοί Νάνοι","Αστέρες: Μαγνητοϋδροδυναμική","ΑΣΤΕΡΕΣ: ΠΕΡΙΣΤΡΟΦΗ","Υπολογιστική αστροφυσική","Computational astrophysics","Numerical methods","Numerical techniques","Stars: Magnetohydrodynamics","STARS: ROTATION","STARS: STRUCTURE","Stars: White Dwarfs","Φυσικές Επιστήμες","Φυσική","Natural Sciences","Physical Sciences"]}]},{"id":"language_rights","label":"Language and Rights","entries":[{"key":"dc:language","label":"Dc Language","values":["gre"]}]},{"id":"identifiers","label":"Identifiers","entries":[{"key":"dc:identifier","label":"Identifier","values":["10.12681/eadd/1748","http://hdl.handle.net/10442/hedi/1748"]}]},{"id":"additional","label":"Additional Metadata","entries":[{"key":"dc:description","label":"Description","values":["THIS THESIS REPRESENTS A THEORETICAL STUDY OF AN EITHER UNIFORM OR NONUNIFORM ROTATION OF A COMPLETELY DEGENERATE ELECTRON GAS CONTINUUM, FORMING A WHITE DWAR. THE AIM OF CHAPTER 1 IS TO SPECIFY THE STRUCTURE DIFFERENTIALLY ROTATING WHITE DWARF BY EXTENDING CHANDRASEKHAR'S METHOD TO INCLUDE UP TO THIRD ORDER TERMS IN THE ROTATIONAL PERTURBATION PARAMETER. IN CHAPTERS II AND III WE OBTAIN NUMERICAL RESULTS THAT PERMIT US THE DETERMINATION OF THE WHITE DWARF STRUCTURE FORUNIFORM ROTATION AND FOR A WEAK, MEDIUM, OR EVEN STRONG DIFFERENTIAL ROTATION.THE RESULTS OBTAINED BY A BOTH SIMPLE AND TIME-SAVING TECHNIQUE ARE THEN COMPARED TO THOSE OF PREVIOUS INVESTIGATIONS, AND THEY ARE FOUND TO BE IN AGREEMENT WITH THEM. THE AIM OF CHAPTER IV IS TO DETERMINE THE STRUCTURE OF A DIFFERENTIALLY ROTATING MAGNETIC WHITE DWARF BY EXTENDING CHANDRASEKHAR'S METHOD TO INCLUDE UP TO SECOND ORDER TERMS IN BOTH THE ROTATIONAL AND THE MAGNETIC PERTURBATIONPARAMETERS. IN CHAPTER V, WE OBTAIN NUMERICAL RESULTS THAT PERMIT US THE DETERMINATION OF THE WHITE DWARF STRUCTURE FOR UNIFORM ROTATION AND FOR A WEAK, MEDIUM OR EVEN STRONG DIFFERENTIAL ROTATION, IN THE PRESENCE OF AN EITHER WEAK OR STRONG MAGNETIC FIELD.","Η ΠΑΡΟΥΣΑ ΔΙΑΤΡΙΒΗ ΑΝΤΙΠΡΟΣΩΠΕΥΕΙ ΜΙΑ ΘΕΩΡΗΤΙΚΗ ΜΕΛΕΤΗ ΣΤΕΡΕΑΣ 'Η ΜΗ ΣΤΕΡΕΑΣ ΠΕΡΙΣΤΡΟΦΗΣ ΠΛΗΡΩΣ ΕΚΦΥΛΙΣΜΕΝΟΥ ΑΕΡΙΟΥ ΗΛΕΚΤΡΟΝΙΩΝ ΜΕ ΤΗΝ ΜΟΡΦΗ ΛΕΥΚΟΥ ΝΑΝΟΥ. Ο ΣΤΟΧΟΣ ΤΟΥ ΚΕΦΑΛΑΙΟΥ Ι ΕΙΝΑΙ Ο ΚΑΘΟΡΙΣΜΟΣ ΤΗΣ ΔΟΜΗΣ ΔΙΑΦΟΡΙΚΑ ΠΕΡΙΣΤΡΕΦΟΜΕΝΟΥ ΛΕΥΚΟΥ ΝΑΝΟΥ, ΔΙΑ ΤΗΣ ΕΠΕΚΤΑΣΗΣ ΤΗΣ ΜΕΘΟΔΟΥ ΤΟΥ CHANDROSEKHAR ΩΣ ΝΑ ΠΕΡΙΛΑΜΒΑΝΕΙ ΟΡΟΥΣ ΜΕΧΡΙ ΚΑΙ ΤΡΙΤΗΣ ΤΑΞΗΣ ΣΤΗΝ ΠΕΡΙΣΤΡΟΦΙΚΗ ΠΑΡΑΜΕΤΡΟ ΔΙΑΤΑΡΑΧΗΣ. ΣΤΑ ΚΕΦΑΛΑΙΑ ΙΙ ΚΑΙ ΙΙΙ ΥΠΟΛΟΓΙΖΟΥΜΕ ΤΑ ΑΡΙΘΜΗΤΙΚΑ ΑΠΟΤΕΛΕΣΜΑΤΑ ΠΟΥ ΜΑΣ ΕΠΙΤΡΕΠΟΥΝ ΤΟΝ ΠΡΟΣΔΙΟΡΙΣΜΟ ΤΗΣ ΔΟΜΗΣ ΤΟΥ ΛΕΥΚΟΥ ΝΑΝΟΥ ΓΙΑ ΤΗΝ ΠΕΡΙΠΤΩΣΗ ΤΗΣ ΣΤΕΡΕΑΣ ΠΕΡΙΣΤΡΟΦΗΣ, ΚΑΙ ΓΙΑ ΤΗΝ ΠΕΡΙΠΤΩΣΗ ΑΣΘΕΝΟΥΣ, ΜΕΤΡΙΑΣ ΚΑΙ ΙΣΧΥΡΗΣ ΔΙΑΦΟΡΙΚΗΣ ΠΕΡΙΣΤΡΟΦΗΣ. ΤΑ ΑΠΟΤΕΛΕΣΜΑΤΑ ΠΟΥ ΕΧΟΥΝ ΠΑΡΑΧΘΕΙ ΑΠΟ ΜΙΑ ΑΠΛΗ ΚΑΙ ΤΑΧΕΙΑ ΑΡΙΘΜΗΤΙΚΗ ΜΕΘΟΔΟ, ΣΥΓΚΡΙΝΟΝΤΑΙ ΜΕ ΑΠΟΤΕΛΕΣΜΑΤΑ ΑΛΛΩΝ ΕΡΕΥΝΗΤΩΝ ΚΑΙ ΑΠΟ ΤΗΝ ΣΥΓΚΡΙΣΗ ΠΡΟΚΥΠΤΕΙ ΟΤΙ ΕΙΝΑΙ ΣΕ ΣΥΜΦΩΝΙΑ ΜΕ ΑΥΤΑ. Ο ΣΤΟΧΟΣ ΤΟΥ ΚΕΦΑΛΑΙΟΥ IV ΕΙΝΑΙ Ο ΠΡΟΣΔΙΟΡΙΣΜΟΣ ΤΗΣ ΔΟΜΗΣ ΔΙΑΦΟΡΙΚΑ ΠΕΡΙΣΤΡΕΦΟΜΕΝΟΥ ΜΑΓΝΗΤΙΚΟΥ ΛΕΥΚΟΥ ΝΑΝΟΥ, ΔΙΑ ΤΗΣ ΕΠΕΚΤΑΣΗΣ ΤΗΣ ΜΕΘΟΔΟΥ ΤΟΥ CHANDRASEKHAR ΩΣΤΕ ΝΑ ΠΕΡΙΛΑΜΒΑΝΕΙ ΟΡΟΥΣ ΜΕΧΡΙ ΚΑΙ ΔΕΥΤΕΡΑΣ ΤΑΞΗΣ ΚΑΙ ΣΤΗΝ ΠΕΡΙΣΤΡΟΦΙΚΗ ΚΑΙ ΣΤΗΝ ΜΑΓΝΗΤΙΚΗ ΠΑΡΑΜΕΤΡΟ ΔΙΑΤΑΡΑΧΗΣ. ΣΤΟ ΚΕΦΑΛΑΙΟ V, ΥΠΟΛΟΓΙΖΟΥΜΕ ΤΑ ΑΡΙΘΜΗΤΙΚΑ ΑΠΟΤΕΛΕΣΜΑΤΑ ΠΟΥ ΜΑΣ ΕΠΙΤΡΕΠΟΥΝ ΤΟΝ ΠΡΟΣΔΙΟΡΙΣΜΟ ΤΗΣ ΔΟΜΗΣ ΤΟΥ ΛΕΥΚΟΥ ΝΑΝΟΥ ΓΙΑ ΤΗΝ ΠΕΡΙΠΤΩΣΗ ΣΤΕΡΕΑΣ ΠΕΡΙΣΤΡΟΦΗΣ ΚΑΙ ΓΙΑ ΤΗΝ ΠΕΡΙΠΤΩΣΗ ΑΣΘΕΝΟΥΣ, ΜΕΤΡΙΑΣ, ΚΑΙ ΙΣΧΥΡΗΣ ΔΙΑΦΟΡΙΚΗΣ ΠΕΡΙΣΤΡΟΦΗΣ, ΠΑΡΟΥΣΙΑ ΑΣΘΕΝΟΥΣ 'Η ΙΣΧΥΡΟΥ ΜΑΓΝΗΤΙΚΟΥ ΠΕΔΙΟΥ."]},{"key":"dc:title","label":"Title","values":["ΣΥΜΒΟΛΗ ΣΤΟ ΠΡΟΒΛΗΜΑ ΤΗΣ ΔΙΑΦΟΡΙΚΗΣ ΠΕΡΙΣΤΡΟΦΗΣ ΕΝΟΣ ΛΕΥΚΟΥ ΝΑΝΟΥ ΜΕ ΑΝΑΠΤΥΞΗ ΚΑΙ ΕΦΑΡΜΟΓΗ ΘΕΩΡΙΩΝ ΔΙΑΤΑΡΑΧΗΣ","CONTRIBUTION TO THE PROBLEM OF DIFFERENTIAL ROTATION OF A WHITE DWARE BY DEVELOPING AND APPLYING PERTURBATION THEORIES"]}]}],"canonical_facts":{"dc:creator":["Hadjopoulos, Anastasios","Χατζόπουλος, Αναστάσιος"],"dc:date":["1991"],"dc:description":["THIS THESIS REPRESENTS A THEORETICAL STUDY OF AN EITHER UNIFORM OR NONUNIFORM ROTATION OF A COMPLETELY DEGENERATE ELECTRON GAS CONTINUUM, FORMING A WHITE DWAR. THE AIM OF CHAPTER 1 IS TO SPECIFY THE STRUCTURE DIFFERENTIALLY ROTATING WHITE DWARF BY EXTENDING CHANDRASEKHAR'S METHOD TO INCLUDE UP TO THIRD ORDER TERMS IN THE ROTATIONAL PERTURBATION PARAMETER. IN CHAPTERS II AND III WE OBTAIN NUMERICAL RESULTS THAT PERMIT US THE DETERMINATION OF THE WHITE DWARF STRUCTURE FORUNIFORM ROTATION AND FOR A WEAK, MEDIUM, OR EVEN STRONG DIFFERENTIAL ROTATION.THE RESULTS OBTAINED BY A BOTH SIMPLE AND TIME-SAVING TECHNIQUE ARE THEN COMPARED TO THOSE OF PREVIOUS INVESTIGATIONS, AND THEY ARE FOUND TO BE IN AGREEMENT WITH THEM. THE AIM OF CHAPTER IV IS TO DETERMINE THE STRUCTURE OF A DIFFERENTIALLY ROTATING MAGNETIC WHITE DWARF BY EXTENDING CHANDRASEKHAR'S METHOD TO INCLUDE UP TO SECOND ORDER TERMS IN BOTH THE ROTATIONAL AND THE MAGNETIC PERTURBATIONPARAMETERS. IN CHAPTER V, WE OBTAIN NUMERICAL RESULTS THAT PERMIT US THE DETERMINATION OF THE WHITE DWARF STRUCTURE FOR UNIFORM ROTATION AND FOR A WEAK, MEDIUM OR EVEN STRONG DIFFERENTIAL ROTATION, IN THE PRESENCE OF AN EITHER WEAK OR STRONG MAGNETIC FIELD.","Η ΠΑΡΟΥΣΑ ΔΙΑΤΡΙΒΗ ΑΝΤΙΠΡΟΣΩΠΕΥΕΙ ΜΙΑ ΘΕΩΡΗΤΙΚΗ ΜΕΛΕΤΗ ΣΤΕΡΕΑΣ 'Η ΜΗ ΣΤΕΡΕΑΣ ΠΕΡΙΣΤΡΟΦΗΣ ΠΛΗΡΩΣ ΕΚΦΥΛΙΣΜΕΝΟΥ ΑΕΡΙΟΥ ΗΛΕΚΤΡΟΝΙΩΝ ΜΕ ΤΗΝ ΜΟΡΦΗ ΛΕΥΚΟΥ ΝΑΝΟΥ. Ο ΣΤΟΧΟΣ ΤΟΥ ΚΕΦΑΛΑΙΟΥ Ι ΕΙΝΑΙ Ο ΚΑΘΟΡΙΣΜΟΣ ΤΗΣ ΔΟΜΗΣ ΔΙΑΦΟΡΙΚΑ ΠΕΡΙΣΤΡΕΦΟΜΕΝΟΥ ΛΕΥΚΟΥ ΝΑΝΟΥ, ΔΙΑ ΤΗΣ ΕΠΕΚΤΑΣΗΣ ΤΗΣ ΜΕΘΟΔΟΥ ΤΟΥ CHANDROSEKHAR ΩΣ ΝΑ ΠΕΡΙΛΑΜΒΑΝΕΙ ΟΡΟΥΣ ΜΕΧΡΙ ΚΑΙ ΤΡΙΤΗΣ ΤΑΞΗΣ ΣΤΗΝ ΠΕΡΙΣΤΡΟΦΙΚΗ ΠΑΡΑΜΕΤΡΟ ΔΙΑΤΑΡΑΧΗΣ. ΣΤΑ ΚΕΦΑΛΑΙΑ ΙΙ ΚΑΙ ΙΙΙ ΥΠΟΛΟΓΙΖΟΥΜΕ ΤΑ ΑΡΙΘΜΗΤΙΚΑ ΑΠΟΤΕΛΕΣΜΑΤΑ ΠΟΥ ΜΑΣ ΕΠΙΤΡΕΠΟΥΝ ΤΟΝ ΠΡΟΣΔΙΟΡΙΣΜΟ ΤΗΣ ΔΟΜΗΣ ΤΟΥ ΛΕΥΚΟΥ ΝΑΝΟΥ ΓΙΑ ΤΗΝ ΠΕΡΙΠΤΩΣΗ ΤΗΣ ΣΤΕΡΕΑΣ ΠΕΡΙΣΤΡΟΦΗΣ, ΚΑΙ ΓΙΑ ΤΗΝ ΠΕΡΙΠΤΩΣΗ ΑΣΘΕΝΟΥΣ, ΜΕΤΡΙΑΣ ΚΑΙ ΙΣΧΥΡΗΣ ΔΙΑΦΟΡΙΚΗΣ ΠΕΡΙΣΤΡΟΦΗΣ. ΤΑ ΑΠΟΤΕΛΕΣΜΑΤΑ ΠΟΥ ΕΧΟΥΝ ΠΑΡΑΧΘΕΙ ΑΠΟ ΜΙΑ ΑΠΛΗ ΚΑΙ ΤΑΧΕΙΑ ΑΡΙΘΜΗΤΙΚΗ ΜΕΘΟΔΟ, ΣΥΓΚΡΙΝΟΝΤΑΙ ΜΕ ΑΠΟΤΕΛΕΣΜΑΤΑ ΑΛΛΩΝ ΕΡΕΥΝΗΤΩΝ ΚΑΙ ΑΠΟ ΤΗΝ ΣΥΓΚΡΙΣΗ ΠΡΟΚΥΠΤΕΙ ΟΤΙ ΕΙΝΑΙ ΣΕ ΣΥΜΦΩΝΙΑ ΜΕ ΑΥΤΑ. Ο ΣΤΟΧΟΣ ΤΟΥ ΚΕΦΑΛΑΙΟΥ IV ΕΙΝΑΙ Ο ΠΡΟΣΔΙΟΡΙΣΜΟΣ ΤΗΣ ΔΟΜΗΣ ΔΙΑΦΟΡΙΚΑ ΠΕΡΙΣΤΡΕΦΟΜΕΝΟΥ ΜΑΓΝΗΤΙΚΟΥ ΛΕΥΚΟΥ ΝΑΝΟΥ, ΔΙΑ ΤΗΣ ΕΠΕΚΤΑΣΗΣ ΤΗΣ ΜΕΘΟΔΟΥ ΤΟΥ CHANDRASEKHAR ΩΣΤΕ ΝΑ ΠΕΡΙΛΑΜΒΑΝΕΙ ΟΡΟΥΣ ΜΕΧΡΙ ΚΑΙ ΔΕΥΤΕΡΑΣ ΤΑΞΗΣ ΚΑΙ ΣΤΗΝ ΠΕΡΙΣΤΡΟΦΙΚΗ ΚΑΙ ΣΤΗΝ ΜΑΓΝΗΤΙΚΗ ΠΑΡΑΜΕΤΡΟ ΔΙΑΤΑΡΑΧΗΣ. ΣΤΟ ΚΕΦΑΛΑΙΟ V, ΥΠΟΛΟΓΙΖΟΥΜΕ ΤΑ ΑΡΙΘΜΗΤΙΚΑ ΑΠΟΤΕΛΕΣΜΑΤΑ ΠΟΥ ΜΑΣ ΕΠΙΤΡΕΠΟΥΝ ΤΟΝ ΠΡΟΣΔΙΟΡΙΣΜΟ ΤΗΣ ΔΟΜΗΣ ΤΟΥ ΛΕΥΚΟΥ ΝΑΝΟΥ ΓΙΑ ΤΗΝ ΠΕΡΙΠΤΩΣΗ ΣΤΕΡΕΑΣ ΠΕΡΙΣΤΡΟΦΗΣ ΚΑΙ ΓΙΑ ΤΗΝ ΠΕΡΙΠΤΩΣΗ ΑΣΘΕΝΟΥΣ, ΜΕΤΡΙΑΣ, ΚΑΙ ΙΣΧΥΡΗΣ ΔΙΑΦΟΡΙΚΗΣ ΠΕΡΙΣΤΡΟΦΗΣ, ΠΑΡΟΥΣΙΑ ΑΣΘΕΝΟΥΣ 'Η ΙΣΧΥΡΟΥ ΜΑΓΝΗΤΙΚΟΥ ΠΕΔΙΟΥ."],"dc:identifier":["10.12681/eadd/1748","http://hdl.handle.net/10442/hedi/1748"],"dc:language":["gre"],"dc:publisher":["University of Patras","Πανεπιστήμιο Πατρών"],"dc:subject":["Αριθμητικές μέθοδοι","Αριθμητικές τεχνικές","ΑΣΤΕΡΕΣ: ΔΟΜΗ","Αστέρες: Λευκοί Νάνοι","Αστέρες: Μαγνητοϋδροδυναμική","ΑΣΤΕΡΕΣ: ΠΕΡΙΣΤΡΟΦΗ","Υπολογιστική αστροφυσική","Computational astrophysics","Numerical methods","Numerical techniques","Stars: Magnetohydrodynamics","STARS: ROTATION","STARS: STRUCTURE","Stars: White Dwarfs","Φυσικές Επιστήμες","Φυσική","Natural Sciences","Physical Sciences"],"dc:title":["ΣΥΜΒΟΛΗ ΣΤΟ ΠΡΟΒΛΗΜΑ ΤΗΣ ΔΙΑΦΟΡΙΚΗΣ ΠΕΡΙΣΤΡΟΦΗΣ ΕΝΟΣ ΛΕΥΚΟΥ ΝΑΝΟΥ ΜΕ ΑΝΑΠΤΥΞΗ ΚΑΙ ΕΦΑΡΜΟΓΗ ΘΕΩΡΙΩΝ ΔΙΑΤΑΡΑΧΗΣ","CONTRIBUTION TO THE PROBLEM OF DIFFERENTIAL ROTATION OF A WHITE DWARE BY DEVELOPING AND APPLYING PERTURBATION THEORIES"],"dc:type":["PhD Thesis"]},"updated_at":"2026-07-24T02:25:05Z"}