Terahertz to Nanohertz

For decades, electronics could generate frequencies up to ~100 GHz and optics could work down to ~10 THz, but the range between 0.1 and 10 THz was hard to reach from either direction. Electronic oscillators became too slow and lasers too low-energy. Only in the last 20 years have quantum cascade lasers and photoconductive antennas started closing this gap, opening new applications in imaging and spectroscopy.

Active scanners illuminate passengers with millimeter or terahertz waves (typically 0.1–1 THz), which pass through clothing but reflect off skin and dense objects. The reflected signal creates a body outline showing concealed items without ionising radiation. Because terahertz energy is about a million times weaker than an X-ray photon, it cannot break chemical bonds or damage DNA.

No. Terahertz photons carry far less energy than visible light photons and are non-ionising — they cannot knock electrons off atoms or damage DNA. At extremely high power they could heat tissue (like a microwave), but every practical terahertz imaging system operates at power levels thousands of times below any thermal threshold. You are bathed in more terahertz radiation from your own body heat than from an airport scanner.

Red light starts around 430 THz (700 nm wavelength) and violet reaches about 750 THz (400 nm). So the entire rainbow occupies roughly 430–750 THz. Infrared sits below red at 0.3–430 THz, and ultraviolet begins above violet at 750+ THz. When someone says "terahertz imaging," they mean the far-infrared end below about 10 THz — well below anything your eyes can detect.

For some applications, yes. Terahertz imaging can distinguish cancerous from healthy tissue based on water-content differences, and it does so without ionising radiation. It is already used experimentally during skin and breast cancer surgery to check tumor margins in real time. The limitation is penetration depth: terahertz waves are absorbed by water within millimeters, so they cannot image deep organs the way X-rays or MRI can.

It sounds absurd, but nanohertz signals are real — they just unfold on geological or cosmic timescales. Pulsar timing arrays detect them by recording tiny shifts in pulsar pulse arrivals over decades. The signal is there the whole time; you simply need a clock patient enough (and stable enough) to notice it. Think of it like tracking the slow wobble of a spinning top filmed over years.

In 2023 NANOGrav announced strong evidence for a gravitational-wave background at roughly 1–100 nHz. The likely source is thousands of supermassive black-hole pairs spiralling toward merger across the universe. Each pair radiates gravitational waves so low-pitched that one full wave cycle can take years to pass through our solar system.

Any conventional oscillator drifts far more than a nanohertz over the time needed to observe one cycle. Millisecond pulsars serve as nature's most stable clocks — their spin is predictable to parts in 10¹⁵. By comparing dozens of these cosmic clocks scattered across the sky, astronomers tease out correlated timing shifts smaller than 100 nanoseconds spread over 15+ years.

The Chandler wobble is a small, slow oscillation of Earth's rotational axis around its figure axis, with a period of about 433 days — roughly 27 nHz. It was discovered by Seth Carlo Chandler in 1891 and is thought to be sustained by pressure fluctuations on the ocean floor. Without it, Earth's axis would settle to a fixed orientation within about 70 years.

Not intentionally. No engineered oscillator is designed to cycle once per decade. However, economic cycles, climate oscillations like El Niño (~50–80 nHz), and solar magnetic-field reversals (~1 nHz) are naturally recurring processes that scientists analyse in the nanohertz band using spectral methods borrowed from signal processing.