Rolling/Slipping Motion of Euler's Disk

We present an experimental study of the motion of a circular disk spun onto a table. With the help of a high speed video system, the temporal evolutions of (i) the inclination angle $\alpha$, (ii) the angular velocity $\omega$ and (iii) the precession rate $\Omega$ are studied. The influence of the...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Caps, H, Dorbolo, S, Ponte, S, Croisier, H, Vandewalle, N
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title
container_volume
creator Caps, H
Dorbolo, S
Ponte, S
Croisier, H
Vandewalle, N
description We present an experimental study of the motion of a circular disk spun onto a table. With the help of a high speed video system, the temporal evolutions of (i) the inclination angle $\alpha$, (ii) the angular velocity $\omega$ and (iii) the precession rate $\Omega$ are studied. The influence of the mass of the disk and the friction between the disk and the supporting surface are considered. %The motions of disks with different masses and over different surfaces are studied. The inclination angle $\alpha$ and the angular velocity are observed to decrease according to a power law. We also show that the precession rate $\Omega$ diverges as the disk stops. Exponents are measured very near the collapse as well as on long range times. Collapsing times have been also measured. The results are compared with previous theoretical and experimental works. The major source of energy dissipation is found to be the slipping of the disk on the plane.
doi_str_mv 10.48550/arxiv.cond-mat/0401278
format Article
fullrecord <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_cond_mat_0401278</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>cond_mat_0401278</sourcerecordid><originalsourceid>FETCH-arxiv_primary_cond_mat_04012783</originalsourceid><addsrcrecordid>eNpjYJA3NNAzsTA1NdBPLKrILNNLzs9L0c1NLNE3MDEwNDK34GRQD8rPycnMS9cPzsksKAAyFHzzSzLz8xTy0xRcS3NSi9SLFVwyi7N5GFjTEnOKU3mhNDeDqptriLOHLtjg-IKizNzEosp4kAXxQAvioRYYE6sOAG7rNWY</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Rolling/Slipping Motion of Euler's Disk</title><source>arXiv.org</source><creator>Caps, H ; Dorbolo, S ; Ponte, S ; Croisier, H ; Vandewalle, N</creator><creatorcontrib>Caps, H ; Dorbolo, S ; Ponte, S ; Croisier, H ; Vandewalle, N</creatorcontrib><description>We present an experimental study of the motion of a circular disk spun onto a table. With the help of a high speed video system, the temporal evolutions of (i) the inclination angle $\alpha$, (ii) the angular velocity $\omega$ and (iii) the precession rate $\Omega$ are studied. The influence of the mass of the disk and the friction between the disk and the supporting surface are considered. %The motions of disks with different masses and over different surfaces are studied. The inclination angle $\alpha$ and the angular velocity are observed to decrease according to a power law. We also show that the precession rate $\Omega$ diverges as the disk stops. Exponents are measured very near the collapse as well as on long range times. Collapsing times have been also measured. The results are compared with previous theoretical and experimental works. The major source of energy dissipation is found to be the slipping of the disk on the plane.</description><identifier>DOI: 10.48550/arxiv.cond-mat/0401278</identifier><language>eng</language><subject>Physics - Soft Condensed Matter ; Physics - Statistical Mechanics</subject><creationdate>2004-01</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/cond-mat/0401278$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.1103/PhysRevE.69.056610$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.cond-mat/0401278$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Caps, H</creatorcontrib><creatorcontrib>Dorbolo, S</creatorcontrib><creatorcontrib>Ponte, S</creatorcontrib><creatorcontrib>Croisier, H</creatorcontrib><creatorcontrib>Vandewalle, N</creatorcontrib><title>Rolling/Slipping Motion of Euler's Disk</title><description>We present an experimental study of the motion of a circular disk spun onto a table. With the help of a high speed video system, the temporal evolutions of (i) the inclination angle $\alpha$, (ii) the angular velocity $\omega$ and (iii) the precession rate $\Omega$ are studied. The influence of the mass of the disk and the friction between the disk and the supporting surface are considered. %The motions of disks with different masses and over different surfaces are studied. The inclination angle $\alpha$ and the angular velocity are observed to decrease according to a power law. We also show that the precession rate $\Omega$ diverges as the disk stops. Exponents are measured very near the collapse as well as on long range times. Collapsing times have been also measured. The results are compared with previous theoretical and experimental works. The major source of energy dissipation is found to be the slipping of the disk on the plane.</description><subject>Physics - Soft Condensed Matter</subject><subject>Physics - Statistical Mechanics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJA3NNAzsTA1NdBPLKrILNNLzs9L0c1NLNE3MDEwNDK34GRQD8rPycnMS9cPzsksKAAyFHzzSzLz8xTy0xRcS3NSi9SLFVwyi7N5GFjTEnOKU3mhNDeDqptriLOHLtjg-IKizNzEosp4kAXxQAvioRYYE6sOAG7rNWY</recordid><startdate>20040116</startdate><enddate>20040116</enddate><creator>Caps, H</creator><creator>Dorbolo, S</creator><creator>Ponte, S</creator><creator>Croisier, H</creator><creator>Vandewalle, N</creator><scope>GOX</scope></search><sort><creationdate>20040116</creationdate><title>Rolling/Slipping Motion of Euler's Disk</title><author>Caps, H ; Dorbolo, S ; Ponte, S ; Croisier, H ; Vandewalle, N</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_cond_mat_04012783</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>Physics - Soft Condensed Matter</topic><topic>Physics - Statistical Mechanics</topic><toplevel>online_resources</toplevel><creatorcontrib>Caps, H</creatorcontrib><creatorcontrib>Dorbolo, S</creatorcontrib><creatorcontrib>Ponte, S</creatorcontrib><creatorcontrib>Croisier, H</creatorcontrib><creatorcontrib>Vandewalle, N</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Caps, H</au><au>Dorbolo, S</au><au>Ponte, S</au><au>Croisier, H</au><au>Vandewalle, N</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Rolling/Slipping Motion of Euler's Disk</atitle><date>2004-01-16</date><risdate>2004</risdate><abstract>We present an experimental study of the motion of a circular disk spun onto a table. With the help of a high speed video system, the temporal evolutions of (i) the inclination angle $\alpha$, (ii) the angular velocity $\omega$ and (iii) the precession rate $\Omega$ are studied. The influence of the mass of the disk and the friction between the disk and the supporting surface are considered. %The motions of disks with different masses and over different surfaces are studied. The inclination angle $\alpha$ and the angular velocity are observed to decrease according to a power law. We also show that the precession rate $\Omega$ diverges as the disk stops. Exponents are measured very near the collapse as well as on long range times. Collapsing times have been also measured. The results are compared with previous theoretical and experimental works. The major source of energy dissipation is found to be the slipping of the disk on the plane.</abstract><doi>10.48550/arxiv.cond-mat/0401278</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier DOI: 10.48550/arxiv.cond-mat/0401278
ispartof
issn
language eng
recordid cdi_arxiv_primary_cond_mat_0401278
source arXiv.org
subjects Physics - Soft Condensed Matter
Physics - Statistical Mechanics
title Rolling/Slipping Motion of Euler's Disk
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-21T20%3A06%3A14IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Rolling/Slipping%20Motion%20of%20Euler's%20Disk&rft.au=Caps,%20H&rft.date=2004-01-16&rft_id=info:doi/10.48550/arxiv.cond-mat/0401278&rft_dat=%3Carxiv_GOX%3Econd_mat_0401278%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true