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Physics: explore STEM content (page 19 of 27) · openstem
Explore STEM Content
Search the community's STEM library — free to study, yours to make your own.
Physics
Mechanics, electromagnetism and quantum on openstem — flashcards, notes, quizzes, plots and sketches shared by the community. Study free, or clone anything into your library.
Name the four fundamental force carriers (gauge bosons) of the Standard Model and the interaction each mediates.1 / 9
Photon (γ) — electromagnetism. Gluon (g) — strong interaction. W± and Z⁰ bosons — weak interaction. (Gravity has no confirmed Standard Model carrier; the hypothesized graviton lies outside the SM.)
What actually happens when you rub a balloon on your hair?
AElectrons move from your hair onto the balloonBThe balloon becomes magneticCNew electrons are created inside the balloonDNothing changes — rubbing has no effect
Oscillations you can change A mass on a spring, a pendulum, a sound wave: they all repeat on a regular cycle. The graph below is a sine wave. Move the sliders and watch what each one controls.
Water has a stretchy skin The very top layer of water behaves differently from the water underneath. Those top molecules pull on each other sideways, making something like a thin stretchy skin across the surface. That's surface tension. It
Three ways a nucleus sheds trouble An unstable nucleus has either too much energy or the wrong neutron-to-proton ratio. It emits something to fix that. Half-life A single nucleus decays at random. A trillion of them decay on a curve you can
Physics
Physics · L4 · Nuclear physics: radioactivity, decay, and binding energy
Equal, opposite, and on two different objects Push on something and it pushes back on you exactly as hard. That's the law. The part people miss is the last clause. Same force, wildly different result A bullet and a recoiling rifle feel forc
What key assumption underlies the FLRW metric, and what does it imply about the universe's large-scale structure?1 / 7
The cosmological principle: on large enough scales, the universe is homogeneous (the same everywhere) and isotropic (the same in every direction). This forces spacetime's spatial geometry to be one of constant curvature, described by a single time-dependent scale factor a(t) and a curvature constant k.
The angle of incidence equals the angle of reflection, both measured from the normal — the line perpendicular to the surface at the point of contact. In symbols, θᵢ = θᵣ.