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Physics · Gravitation and the universe · Grade 9

Scales of the universe

From quarks to the Universe: which laws of physics rule at each scale?

Open the experiment

The situation

Imagine a person standing near the Tashkent TV Tower. If the camera moves away 10 times farther with each step, after 7 steps the whole Earth is visible, and after 21 steps the Milky Way galaxy. If the camera goes inwards, we see a cell, DNA, an atom, a nucleus and the quarks inside a proton. Over the whole journey the scale changes by about 10⁴² times. Are the laws of physics the same at every scale, or does each scale have its own “ruling” law?

Topic

Physical picture of the universe: scales. From a quark to a galaxy: a journey through the powers of ten

Key ideas

  • Powers of ten
  • Fundamental constants
  • Branches of physics

Formulas

lP=ℏGc3≈1.6⋅10−35 m,tP=lPc≈5.4⋅10−44 s

The Planck length and time — a scale built from three fundamental constants.

Rs=2GMc2,λC=hmc

Two limits: if a body is smaller than Rs, it is a black hole; at scales smaller than λC, quantum effects dominate.

(vc)2,ℏmvL,GMrc2

Dimensionless numbers: if they are smaller than the required accuracy, classical (Newtonian) physics is enough.

r→=xi→+yj→+zk→,v→=dr→dt,s=∫t1t2|v→|dt

Reference frame: the position vector, its derivative is the velocity, and the integral of the velocity is the distance travelled.

t=Lc:1.496⋅1011 m3.00⋅108 m/s≈499 s

The speed of light is finite: when we look far away, we see the past.

Theory

Powers of ten: space and time

The diameter of a proton is ≈ 1.7·10⁻¹⁵ m, and the diameter of the observable Universe is ≈ 8.8·10²⁶ m. Such numbers are convenient to write with powers of ten: each step is a factor of 10. Time is the same: light crosses a proton in ≈ 6·10⁻²⁴ s, while the age of the Universe is ≈ 4.4·10¹⁷ s (13.8 billion years). Units of length are chosen according to the scale: fm (nuclei), nm (molecules), m, km, AU (Earth–Sun), the light-year and the parsec (stars), Mpc (galaxies). Space and time are the stage of all phenomena; special relativity unites them into a single space-time.

Reference frame and position vector

To say where a body is, you need a reference frame: a reference body, coordinate axes and a clock. In the “Powers of ten” scene, at the scale of 10² m, the origin is at the foot of the TV tower: x points east, y up, z south. The person's position is the position vector r→=(−120; 0; 80) m. The derivative of the position vector with respect to time is the velocity, and the integral of the velocity is the distance travelled. Velocity depends on the reference frame: a “stationary” person in Tashkent moves at ≈ 350 m/s with the Earth's rotation, at ≈ 30 km/s with the Earth around the Sun, and at ≈ 230 km/s with the Sun around the centre of the Galaxy.

The four interactions: a single picture of the world

All phenomena are explained by four interactions. The strong one holds quarks in protons and neutrons and nucleons in the nucleus; its range is ≈ 10⁻¹⁵ m. The weak one governs β-decay and the first stage of fusion in the Sun; ≈ 10⁻¹⁸ m. The electromagnetic one gives atoms, molecules, chemistry, biology, friction and elasticity; its range is infinite. Gravity is the weakest (≈ 10³⁶ times weaker than the electric repulsion between two protons), but because matter is usually electrically neutral, it dominates at large scales — planets, stars, galaxies. The history of physics is a history of unification: electricity and magnetism (Maxwell), electromagnetic and weak interactions (electroweak theory), the Standard Model; uniting gravity with quantum physics is still unsolved.

The cube of theories: the limits of classical physics

Each theory can be marked by three constants. In the limit c→∞, ℏ→0, G→0 — Newtonian mechanics. When v approaches the speed of light — special relativity; when the action (mvL) is close to ℏ — quantum mechanics; both together — quantum field theory; strong gravity and c — general relativity. Which theory is needed also depends on the accuracy: for GPS clocks even corrections of 10−10 matter, while for a football 1 % accuracy is enough. The old theory remains the limiting case of the new one — this is the correspondence principle.

The microworld: milestones of atomism and particle physics

The size of an atom is ≈ 10⁻¹⁰ m (the Bohr radius is 5.29·10⁻¹¹ m), while the nucleus is ≈ 10⁻¹⁵ m — about 100 000 times smaller than the atom, yet it holds more than 99.9 % of the mass. The microworld is governed by fundamental constants: the elementary charge e, the electron mass me, Planck's constant h, and the speed of light c. The quantum (wave nature, spin, energy levels) and relativistic (antiparticles, E=mc2) properties of particles appear together at this scale. Milestones: the electron (1897, J. J. Thomson), the nucleus (1911, E. Rutherford), the neutron and positron (1932), the quark model (1964), quarks “seen” in experiment (1968–1969, SLAC), W and Z bosons (1983, CERN), the top quark (1995), the Higgs boson (2012, LHC).

Physics, other sciences and society; the model

Physics studies the most general laws of nature through observation, experiment, models and theory; its language is mathematics. It is the foundation of chemistry (the structure of atoms and molecules), biology and medicine (biophysics, X-rays, MRI, PET), geology, astronomy and engineering. Electricity grids, the transistor and computers, lasers, GPS, nuclear power stations and solar panels are products of discoveries in physics; they have transformed society's productive forces. Model: sizes are approximate; the Moon and planets are enlarged to be visible; galaxies and the cosmic web are schematic; the positions of the TV tower and the person are arbitrary.

Did you know?

  • The Tashkent TV Tower is 375 m tall. It was put into operation on 15 January 1985 and from 1985 to 1991 was the fourth tallest tower in the world.
  • A “stationary” person beside the TV tower moves with the Earth's rotation at about 350 m/s — faster than the speed of sound.

Inside the experiment

The experiment starts from a real-life situation: you predict the result, change the controls, run the experiment and draw a conclusion. Inside are missions, theory, a quiz and a guided tour in which the camera moves and explains the key points.

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