Why Science Says Cold Has A Hard Limit Even If The Universe Is Infinite
Astronomy

Why Science Says Cold Has A Hard Limit Even If The Universe Is Infinite

Absolute zero sets an ultimate limit on cold. Discover why cosmic radiation continues to cool and if the universe can ever truly reach zero kelvin.

By Aisha Ahmed
Published:
Email this Article
A frost-covered conceptual thermometer points near absolute zero, −273.15°C, the lowest possible temperature. (CREDIT: The Brighter Side of News)

We rely on freezers to preserve food and industrial cryogenics to push the boundaries of physics, but a fundamental question persists: why can’t we simply keep cooling things indefinitely? While our number system stretches toward negative infinity, the physical reality of temperature is governed by a strict, non-negotiable floor known as absolute zero.

Set at −273.15 degrees Celsius (−459.67 degrees Fahrenheit), or 0 kelvin, absolute zero represents the state where a system reaches its minimum possible energy. Contrary to popular belief, it does not imply a total cessation of all activity. Instead, it marks the point where thermal energy—the chaotic, heat-driven movement of atoms—is entirely stripped away, leaving only the fundamental quantum motion inherent to the ground state.

A freezer turns water into ice. Laboratory refrigerators go much colder.
A freezer turns water into ice. Laboratory refrigerators go much colder. (CREDIT: Shutterstock)

The Physics of the Energy Floor

To understand why cooling stops at this threshold, one must view temperature as an energy extraction process. A refrigerator works by moving energy from an interior space to the warmer surroundings; it does not “inject” cold. By removing thermal energy, a system is nudged closer to its ground state. However, quantum mechanics dictates that a system can only exist in permitted energy states. Just as you cannot descend a staircase that has no steps below the bottom, a refrigerator cannot extract energy from a system that has already reached its lowest allowable state.

This reality was first hinted at by 18th-century physicist Guillaume Amontons, who observed that the pressure of a gas drops as it cools. By plotting these trends, scientists extrapolated that pressure would theoretically hit zero at a specific temperature. Later, Lord Kelvin formalized this into the absolute temperature scale we use today. While exotic “negative temperature” states can be achieved in specialized lab environments, these systems actually represent a population inversion—where higher energy states are more occupied than lower ones—making them technically hotter, not colder, than any positive-temperature system.

Picture a staircase with a bottom step. Descending brings someone closer to that step.
Picture a staircase with a bottom step. Descending brings someone closer to that step. (CREDIT: Shutterstock)

The Unattainability Principle

Even though we know where the boundary sits, the third law of thermodynamics creates a barrier to reaching it. Through finite physical processes, it is impossible to extract the final remnants of entropy to reach 0 K. We can approach it with incredible precision, as evidenced by researchers using ultracold atoms or the James Webb Space Telescope’s Mid-Infrared Instrument, which operates below 7 K, but we can never arrive at the destination.

Interestingly, the universe itself is engaged in a massive cooling operation. The expansion of space acts as a cosmic refrigerator, stretching the wavelengths of the cosmic microwave background (CMB). As the fabric of space expands, the energy of these photons decreases, effectively lowering the background temperature of the cosmos. Yet, even in this grand expansion, the temperature asymptotically approaches zero without ever touching it. Every time the universe doubles in size, the temperature halves, but like the mathematical paradox of Zeno’s arrow, the distance to the floor remains unbridged.

A conceptual illustration shows how cooling contracts the air inside a balloon, while warming allows it to expand.
A conceptual illustration shows how cooling contracts the air inside a balloon, while warming allows it to expand. (CREDIT: Dungrela Publishing)

A Complex Future

The long-term thermal fate of the universe is further complicated by the presence of dark energy. Research by Gary Gibbons and Stephen Hawking suggests that an accelerating universe creates a cosmic event horizon, which carries its own inherent temperature. If dark energy remains constant, the universe may not fade into a absolute-zero void, but rather stabilize at a low, nonzero temperature dictated by this horizon.

While heating theoretically lacks a known ceiling—at least until we reach the enigmatic Planck temperature where current physics breaks down—cold has a definitive, iron-clad boundary. We live in a universe where the floor is fixed, but the path toward it is infinite, ensuring that while the cosmos may continue to grow colder, it will never be truly “finished” with the process.

MIRI, (Mid InfraRed Instrument), flight instrument for the James Webb Space Telescope, JWST, during ambient temperature alignment testing in RAL Space's clean rooms at STFC's Rutherford Appleton Laboratory.
MIRI, (Mid InfraRed Instrument), flight instrument for the James Webb Space Telescope, JWST, during ambient temperature alignment testing in RAL Space’s clean rooms at STFC’s Rutherford Appleton Laboratory. (CREDIT: JWST MIRI)
This map of the Cosmic Microwave Background radiation, imprinted on the sky when the universe was 370,000 years old, shows tiny temperature fluctuations that correspond to regions of slightly different densities.
This map of the Cosmic Microwave Background radiation, imprinted on the sky when the universe was 370,000 years old, shows tiny temperature fluctuations that correspond to regions of slightly different densities. (CREDIT: ESA and the Planck Collaboration)
Fact Checked

This article has been fact checked for accuracy, with information verified against reputable sources. Learn more about us and our editorial process.

Last reviewed on .

Article history

  • Latest version

Reference(s)

  1. Gibbons, G. W.., et al. “Cosmological event horizons, thermodynamics, and particle creation.” Physical Review D, vol. 15, no. 10, May 15, 1977, pp. 2738-2751. American Physical Society (APS), doi: 10.1103/PhysRevD.15.2738. <https://journals.aps.org/prd/abstract/10.1103/PhysRevD.15.2738>.

Cite this page:

Ahmed, Aisha. “Why Science Says Cold Has A Hard Limit Even If The Universe Is Infinite.” BioScience. BioScience ISSN 2521-5760, 04 November 2026. <https://www.bioscience.com.pk/en/subject/astronomy/why-cold-has-a-limit-even-if-the-universe-does-not>. Ahmed, A. (2026, November 04). “Why Science Says Cold Has A Hard Limit Even If The Universe Is Infinite.” BioScience. ISSN 2521-5760. Retrieved November 04, 2026 from https://www.bioscience.com.pk/en/subject/astronomy/why-cold-has-a-limit-even-if-the-universe-does-not Ahmed, Aisha. “Why Science Says Cold Has A Hard Limit Even If The Universe Is Infinite.” BioScience. ISSN 2521-5760. https://www.bioscience.com.pk/en/subject/astronomy/why-cold-has-a-limit-even-if-the-universe-does-not (accessed November 04, 2026).
End of the article