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dc.date.accessioned2020-04-20T19:52:06Z
dc.date.available2020-04-20T19:52:06Z
dc.date.created2019-03-19T17:58:27Z
dc.date.issued2019
dc.identifier.citationKersting, Magdalena . Free fall in curved spacetime—how to visualise gravity in general relativity. Physics Education. 2019, 54(3), 1-9
dc.identifier.urihttp://hdl.handle.net/10852/74677
dc.description.abstractThe first direct observation of gravitational waves in 2015 has led to an increased public interest in topics of general relativity (GR) and astronomy. Physics teachers and educators respond to this interest by introducing modern ideas of gravity and spacetime to high school students. Doing so, they face the challenge of finding suitable models that visualise gravity as the geometry of curved spacetime. Most models of GR, such as the popular rubber sheet model, only address spatial curvature. Yet, according to Albert Einstein, gravitational phenomena stem from deformations both in space and time. This paper presents a new model that builds on a relativistic generalisation of Newton's first law. We use Einstein's free fall thought experiment and a classical height-time diagram to explain how warped time gives rise to gravity. Our warped-time model acts as a convenient supplement to the rubber sheet model. To support teachers in integrating the model into their classroom practice, we have implemented the model as an interactive simulation that is freely accessible. The model is the result of a three-year period of developing and trialling digital learning resources in Norwegian high schools. Based on these trials, we suggest specific instructional strategies on how to use the warped-time model successfully in science classrooms.
dc.languageEN
dc.rightsAttribution 3.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/
dc.titleFree fall in curved spacetime—how to visualise gravity in general relativity
dc.typeJournal article
dc.creator.authorKersting, Magdalena
cristin.unitcode185,15,4,5
cristin.unitnameFysikkdidaktikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1686104
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physics Education&rft.volume=54&rft.spage=1&rft.date=2019
dc.identifier.jtitlePhysics Education
dc.identifier.volume54
dc.identifier.issue3
dc.identifier.doihttps://doi.org/10.1088/1361-6552/ab08f5
dc.identifier.urnURN:NBN:no-77773
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0031-9120
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/74677/4/Kersting_2019_Phys._Educ._54_035008.pdf
dc.type.versionPublishedVersion
cristin.articleid035008
dc.relation.projectNFR/246723


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Attribution 3.0 Unported
This item's license is: Attribution 3.0 Unported