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Primordial Sound Waves Still Shape the Distribution of Galaxies

Caroline ShawMark WhittleAnder MikalsonTEDThursday, September 17, 20264 min read

Astronomer Mark Whittle argues that the cosmic microwave background preserves the pressure waves that moved through the universe’s primordial gas, and that their harmonic structure remains detectable in the later clustering of galaxies. These baryon acoustic oscillations froze when the universe became transparent about 400,000 years after its birth, leaving a measurable link between quantum-scale fluctuations and the large-scale distribution of matter. Whittle’s collaboration with sound artist Ander Mikalson and composer Caroline Shaw turns a deliberately altered sonification of those data into a choral work.

The first cosmic pressure waves still structure the galaxy map

Mark Whittle describes the faint pattern in the cosmic microwave background as more than a picture of the early universe. Its peaks and troughs are the record of pressure waves in primordial gas, and their harmonic pattern survives—faintly but measurably—in the later distribution of galaxies.

The relevant transition came when the universe was about 400,000 years old. Until then, Whittle says, hot gas oscillated under the competing effects of gravity and pressure. As the cooling universe became transparent, those oscillations ceased and their pattern froze in place. Matter subsequently collapsed under gravity to form stars and galaxies, carrying forward an imprint of that earlier acoustic structure.

A mottled CMB field spanning 10 degrees by 10 degrees, or about 8 million light-years, is paired with a Sloan Digital Sky Survey map spanning 4 billion light-years and containing roughly 100,000 galaxies. Wave analysis identifies a faint fundamental and higher harmonics in the web-like galaxy clustering: baryon acoustic oscillations.

What is shownScaleWhat the analysis identifies
Cosmic microwave background patch8 million light-yearsTemperature and pressure peaks and troughs in primordial gas
Sloan Digital Sky Survey galaxy map4 billion light-years; about 100,000 galaxiesA faint fundamental and harmonics in galaxy clustering
The early microwave-background pattern and the later galaxy distribution carry related harmonic structure.

The sound waves have turned to stone, so to speak, and become fossilized in the patterns of galaxies.

Mark Whittle · Source

Whittle places this sequence within a longer causal chain. Subatomic quantum vibrations during inflation—a very brief period of hyper-expansion at the universe’s birth—were, he says, amplified into enormous pressure waves and eventually into the large-scale tapestry of galaxies. In that account, fluctuations smaller than atoms became structures on cosmic scales, connecting quantum processes to the visible distribution of matter.

The microwave background is a measurable acoustic record, not an audible bang

Mark Whittle says the cosmic microwave background reaches Earth from every direction because looking far enough into space means looking back to the universe before galaxies formed. At that time, the universe was an almost uniform hot gas of atomic nuclei and electrons immersed in intense light. Expansion stretched that light from micron-scale wavelengths to millimeter-scale microwaves, which is why it now arrives as the CMB.

The CMB's nearly uniform full-sky brightness gave way, under more sensitive microwave observations, to a map of tiny mottled variations. In a 10-degree-by-10-degree field spanning about 8 million light-years, those variations show the universe at an age of 400,000 years.

The brighter and darker regions reflect slight differences in temperature and pressure in the glowing primordial gas. They are the peaks and troughs of immense pressure waves. Their contrast amounts to 90 decibels, or rock-concert loudness in Whittle’s comparison, but their scale puts their pitch 50 octaves below human hearing; one wave could take 50,000 years to pass.

90 decibels
brightness contrast associated with the primordial acoustic pattern

Gravity, rather than an instantaneous “bang,” drove the sound. Slightly denser regions exerted stronger gravitational pull, drawing in neighboring gas. The gas compressed, rebounded, and fell back inward, producing approximately spherical oscillations. Because the early universe contained regions of different sizes, it supported a range of pitches, like organ pipes of different lengths.

The displayed acoustic-power spectrum contains a fundamental peak and several harmonics. Whittle compares its overall shape with the spectrum of a flute playing a single note: each has a fundamental and harmonics, though they arise for different reasons. The comparison does not make the primordial signal conventionally musical. The cosmic harmonics are broad rather than sharply defined, so an audible rendering sounds more like noise than a clean tone.

A smooth green curve through the measured spectrum represents a detailed computer calculation intended to include the relevant physics. Whittle calls the fit “amazingly good” and says that matching such calculations to the observations measures many fundamental properties of the universe accurately. The spectrum is therefore not merely an analogy to sound; it is part of a quantitative account of the young universe.

Making the pattern audible requires choices that make it musical

Mark Whittle shifts the cosmic spectrum up by 50 octaves before playing it, then tracks the changing harmonics from the Big Bang through the end of the 400,000-year acoustic era. Compressing that history into 10 seconds produces a falling pitch. As time passed, larger regions had time to begin oscillating; their larger waves lowered the overall pitch.

A second sonification makes a further alteration. Whittle identifies when each upshifted harmonic matches notes on a simple piano keyboard. The graph maps descending harmonic tracks against the keyboard over the first 400,000 years. This procedure narrows broad harmonic bands into individual notes and sounds those notes at particular times. A 150,000-year interval, compressed into 10 seconds, consequently has melody and rhythm that the raw cosmic spectrum lacks.

He gave those sequences to Ander Mikalson, who worked with Caroline Shaw, a Pulitzer Prize-winning composer, on a work for choir and organ lasting about 10 minutes. The work has been performed several times; the performance excerpt shown was recorded at the Catholic Cathedral in Richmond, Virginia.

Whittle calls the result a genuine convergence of science and art within a sacred context. He connects that artistic experience to a physical continuity: particles and atoms in the early acoustic gas later became part of stars, galaxies, planets and people.

Those particles and atoms from that first acoustic era went on to make stars and galaxies and planets and, of course, us.

Mark Whittle

Whittle’s final proposition is that human sentience may be an exceedingly rare, perhaps unique, way for the universe to witness and understand its own history.

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