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Hidden Dimensions in the Glow of an Ancient Explosion

Original: "First Search for Kaluza-Klein Gravitons and Radion Using Planck Data"
arXiv:2607.02651v1 · 2026-07-02 · CC BY 4.0 · ⏱ 2 min · Cosmology HEP Theory
Scientists examined the cosmic microwave background for hints of extra dimensions.
Abstract

Возможно, у пространства есть скрытые измерения, похожие на потайные комнаты. Во время быстрого расширения Вселенной (инфляции) эти измерения могли бы создавать небольшие «складки» в распределении вещества. Анализ данных спутника «Планк» не показал таких складок, но некоторые модели предсказывают, что будущие наблюдения смогут их увидеть. Не услышим ли мы когда-нибудь эхо невидимых миров?

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In the first moments after the Big Bang, the universe was incredibly hot and expanding rapidly. Thanks to the work of Georges Lemaître and Edwin Hubble, we know that expansion continues to this day. And in 1965, Arno Penzias accidentally discovered the echo of those events — a faint glow called the cosmic microwave background. It carries the imprints of processes that raged in the cradle of the cosmos.

Imagine ripples on a pond: their pattern can reveal what lies on the bottom. Similarly, physicists study the 'ripples' of ancient light, hoping to spot traces of hidden dimensions.

To peer beyond the familiar world, scientists used a method reminiscent of spectroscopy — typically employed to determine the composition of stars from their light. Here, they searched the cosmic microwave background for special patterns that might betray the existence of particles from other dimensions. Such searches rely on the uncertainty principle and the phenomenon of superposition, which allow particles to briefly appear from the vacuum. Moreover, effects like quantum entanglement and time dilation in the expanding space can alter the expected picture. All of this goes far beyond the Standard Model — our best description of the world of elementary particles.

Analysis of data from the Planck satellite showed no unequivocal signal, but placed strict limits. In other words, if extra dimensions exist, their influence must be very weak. This is important for theories linking dark matter to multidimensional particles, and for understanding how gravitational waves might have been generated in the early universe. Even the growth of entropy — a measure of disorder — helps build such models. And the cosmic microwave background itself, traveling at the speed of light, remains an ideal messenger, bringing us news from the depths of time.

🎯 If you turn on an old analog TV to an empty channel, about 1% of the 'snow' on the screen is noise from the [tag:big_bang]cosmic microwave background[/tag].

🎬 In Greg Egan's novel 'Schild's Ladder', the characters travel through extra dimensions. Our reality is more modest, but the search for traces of hidden worlds in ancient light is like the first steps into that same uncharted territory.

\mu = \sqrt{\frac{M^2}{H^2} - \frac{9}{4}}
If μ ≲ 1, the particle is produced efficiently; for large μ, exponential suppression occurs—this is how the quantum-mechanical filter works.
f_{\rm NL} \sim -\frac{10 M}{3 H^4} \frac{c_g^2 \dot{\sigma}_0}{2 \Lambda_c^2} S_{\rm max}
Here M is the UV physics scale, c_g is the coupling constant, Λc is the confinement scale, Smax is the maximum form factor. The formula links the fundamental model parameters to the observable quantity.
Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
big bang Standard Model dark matter spectroscopy gravitational waves uncertainty principle superposition quantum entanglement speed of light Time dilation entropy
Laws
Friedmann equationsHubble's lawsecond law of thermodynamicsSchrödinger equationDoppler effectHeisenberg uncertainty principle
Original: arXiv:2607.02651v1 · CC BY 4.0 · bridge42worlds