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Seventeen particles, one room — yours

I'm not a physicist — that's the point. The method, run where I hold no credential. Every number computes in your browser; every derivation is shown below.

The chart — everything you are is generation one · click any tile

gen 1 — you
gen 2
gen 3
forces · mass
the chart is a map, not a container — lit jumps to its instrument, work highlights its line, never answers honestly, queued tells you when.

loading the chart state…

The instruments — in your browser, from your clock; nothing leaves your tab

01
μ

What's raining through you right now?

Born 15 km up, 2.2 μs to live — dead in 660 m, by the math. From your seat they arrive because their clocks tick slow; from the muon's seat its clock is fine — it's the atmosphere that length-contracts to a few hundred meters. Two stories, one arrival: that agreement is special relativity. Its heavier sibling, the tau, never makes it.

1.1muons / cm²·min at sea level · PDG
in the muon's own frame it still lives just 2.2 μs. what saves it?
02
e

You are a decay engine.

Potassium-40 and carbon-14 decay inside you, every second of your life. Harmless — a night beside another human adds ~0.05 μSv. You have always been a source.

every tick is a W boson at work · how we know →
about 7,400decays / second inside you · UNSCEAR
a running count of decays since you opened this page
03
ν

What's pouring through your thumbnail?

Born νe in the Sun's core, gone instantly — the light beside them takes 100,000 years to get out. By your thumbnail the river is all three flavors: Davis was "wrong" for 30 years, until oscillation proved neutrinos have mass — the Standard Model's first crack. One river, three slots, honestly.

runs on the W · first seen via the Z · how we know →
through 1 cm² since you arrived · ~65 billion /cm²·s
assuming 40°N — set yours
Almost certainly zero — a lifetime total of one or two. So how did anyone ever detect one? That question built Super-Kamiokande. the derivation →
04
γ

The oldest light is in the room with you.

The cosmic microwave background: 13.8 billion years in flight, arriving from every direction — famously, roughly a percent of analog static. Its discoverers spent a year blaming pigeons; the hiss stayed. Ruling out is the method.

411CMB photons in every cm³ of your room
Animated static; about one percent of the flicker represents cosmic microwave background photons.
05
g

Your mass is mostly trapped energy.

Zoom from your body to the inside of a proton. The quarks' own masses cover barely 1% — the rest is the energy of confinement. Nuclear binding energy subtracts; confinement traps. Trapped energy weighs.

the 1% that isn't glue is the Higgs — the electron's mass sets every atom's size · the budget →

Met by their work · honestly never — one true thing each

The arithmetic — how we know, in five short sums

μ

Why any muon reaches you at all

At rest a muon lives τ = 2.2 μs — at light speed that is a range of

c·τ = 3×10⁸ m/s × 2.2×10⁻⁶ s ≈ 660 m

far short of the ~15 km of atmosphere. But a typical ~4 GeV sea-level muon carries γ = E/mc² ≈ 4000/105.7 ≈ 38, so from your frame its clock runs 38× slow: range ≈ 38 × 660 m ≈ 25 km. From the muon's frame the same γ contracts the 15 km of sky to ~400 m. Both frames predict arrival — that agreement is the theory.

inputs: PDG muon mass 105.7 MeV, mean sea-level muon energy ~4 GeV, flux ~1 /cm²·min

e

Your ~7,400 Bq, from scratch

A 70 kg body holds ~140 g potassium (0.2% of mass). K-40 is 0.0117% of that: 16 mg → N ≈ 2.5×10²⁰ atoms. With half-life 1.25 Gy:

A = N·ln2/t½ ≈ 2.5×10²⁰ × 0.693 / (3.9×10¹⁶ s) ≈ 4,400 Bq

Carbon-14 (1.2 parts per trillion of your ~16 kg carbon, t½ 5,730 y) adds ~3,000 Bq. Total ≈ 7,400 decays every second — about 106 per kg, which is what the slider computes.

inputs: UNSCEAR body composition; K-40 t½ 1.25×10⁹ y; C-14 t½ 5,730 y

ν

65 billion through every cm², from sunlight alone

The pp chain releases 26.7 MeV and exactly 2 neutrinos per helium made. The Sun's power is 3.8×10²⁶ W, so it must emit

2 × 3.8×10²⁶ / 4.3×10⁻¹² J ≈ 1.8×10³⁸ ν/s

Spread over a sphere of radius 1 AU (4πr² ≈ 2.8×10²⁷ cm²): ≈ 6.5×10¹⁰ per cm² per second. You can derive the flux from nothing but the solar constant — the detection story is the hard part, and it's why the "how many stopped inside you?" answer built Super-Kamiokande.

inputs: solar luminosity 3.8×10²⁶ W; pp-chain 26.7 MeV; 1 AU = 1.5×10¹³ cm

γ

411 ancient photons per cm³

A blackbody at temperature T holds a fixed photon density. For the CMB's measured T = 2.725 K:

n = (2ζ(3)/π²) (kT/ħc)³ ≈ 411 photons/cm³

No fitting, no cosmology dial — one measured temperature in, one room-filling number out. The "about a percent of analog static" claim is looser: it depends on the receiver, which is why the page hedges it.

inputs: COBE/FIRAS T = 2.725 K; ζ(3) ≈ 1.202

g

The 1% quark, 99% glue budget

A proton weighs 938.3 MeV. Its three valence quarks weigh

2×m(u) + m(d) ≈ 2×2.2 + 4.7 ≈ 9.1 MeV ≈ 1%

The other ~99% is QCD binding — confinement energy, carried by the gluon field. Nuclear binding energy makes nuclei lighter than their parts; confinement makes the proton heavier than its quarks. Different signs, both "trapped energy weighs."

inputs: PDG quark masses (MS-bar); proton mass 938.272 MeV

sources: PDG · Bahcall · UNSCEAR · COBE/FIRAS · long-form derivation notes land under the cosmos tag, one per instrument
chart state: data/particles.json · owned by gen_particles.py · your quiz ring stays in your browser
queued next: up/down quark instrument · share-card of your numbers · Geiger click