A comprehensive modelling and experimental approach for damped oscillations in U-tubes via Easy JavaScript Simulations

Bibcode
2023PhyEd..58e5007O
DOI
10.1088/1361-6552/acdb27
Orjuela, Fredy A.; García-Farieta, J. E.; Hortúa, Héctor J.; Munévar, E.
Referencia bibliográfica

Physics Education

Fecha de publicación:
9
2023
Revista
Physics Education
Número de autores
4
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
In recent years, science simulations have become popular among educators due to their educational usefulness, availability, and potential for increasing the students' knowledge on scientific topics. In this paper, we introduce the implementation of a user-friendly simulation based on Easy Java/JavaScript Simulations (EJS) to study the problem of damped oscillations in U-tubes EJS. Furthermore, we illustrate various advantages associated with the capabilities of EJS in terms of design and usability in order to encourage teachers to use it as an educational supplement to physics laboratories .
Tipo
Con árbitro

Te puede interesar

  • Con árbitro
    Beyond the Nyquist frequency: Asteroseismic catalog of undersampled Kepler late subgiants and early red giants
    Subgiants and early red giants are crucial for studying the first dredge-up, a key evolutionary phase in which the convective envelope deepens, mixing previously interior-processed material and bringing it to the surface. Yet, very few have been seismically characterized with Kepler because their oscillation frequencies are close to the 30 minute
    Liagre, B. et al.

    Fecha de publicación:

    10
    2025
    Bibcode
    2025A&A...702A.144L
    Número de citas
    0
  • Con árbitro
    An ALMA Band 7 survey of SDSS/Herschel quasars in Stripe 82: I. The properties of the 870 micron counterparts
    Context. Over the past 15 years, studies of quasars in the far-infrared (FIR) have reported host luminosities ranging from 10 12 to 10 14 L ⊙. These luminosities, often derived from Herschel/SPIRE photometry, suggest star formation rates (SFRs) of up to several thousand M ⊙ yr ‑1, positioning them among the most luminous starburst galaxies in the
    Hatziminaoglou, E. et al.

    Fecha de publicación:

    10
    2025
    Bibcode
    2025A&A...702A.183H
    Número de citas
    0
  • Con árbitro
    Transit timing variations in HIP 41378: CHEOPS and TESS confirm a non-transiting sixth planet in the system
    In multiple-planet systems, gravitational interactions of exoplanets could lead to transit timing variations (TTVs), whose amplitude becomes significantly enhanced when planets are in or near mean-motion resonances (MMRs), making them more easily detectable. In cases where both TTVs and radial velocity (RV) measurements are available, combined
    Leonardi, P. et al.

    Fecha de publicación:

    10
    2025
    Bibcode
    2025A&A...702A.211L
    Número de citas
    0