BUCKYVERSE

Purdue Ultrawhite Radiative Cooling Paint

Overview

Purdue University researchers developed BaSO4 (barium sulfate) nanoparticle acrylic paint achieving 98.1% solar reflectance — the whitest paint ever created — designed for passive radiative cooling of buildings without electricity.

Cooling Mechanism

The paint cools through two complementary processes:

  1. Reflecting incoming solar radiation (0.3-2.5 μm wavelengths)
  2. Emitting infrared heat through Earth's atmospheric transparency window (8-13 μm) directly to outer space

Unlike typical white paints that absorb and retain heat, this formulation maintains surfaces below ambient temperature even during daytime.

Material Composition

Particle Geometry — The Key Innovation

The paint contains BaSO4 nanoparticles with deliberately varied sizes. This heterogeneous distribution is critical:

Performance Data

Metric Value
Solar reflectance 98.1% (vs. 80-90% commercial, 95.5% prior CaCO3 formulation)
Sky window emissivity 0.95
Average cooling power 117 W/m²
Daytime cooling (noon sun) 8°F (4.4°C) below ambient
Nighttime cooling 19°F (10.6°C) below ambient
Winter cooling (43°F ambient) 18°F reduction
Roof cooling power (1,000 sq ft) ~10 kW — equivalent to or exceeding typical residential AC

Practical Considerations

Broader Context — Radiative Cooling Materials Landscape

Four dominant technology clusters for passive radiative cooling (per 2026 patent landscape):

  1. Metamaterial nanostructured emitters: Metal-plated tapered nanopores via anodic aluminum oxide (PARC); near-unity emissivity
  2. Polymer/particle composite films: Fluoropolymers, PDMS, or polyethylene loaded with TiO2, SiO2, CaCO3, SiC, ZnO, Al2O3
  3. Photonic multilayer stacks: Alternating dielectric layers (HfO2/SiO2) engineering spectrally selective properties
  4. Vacuum-insulated far-infrared radiators: ≥0.80 emissivity in 8-13 μm band

Emerging frontier: radiative cooling engines (modified Stirling) converting surface-to-sky temperature difference into electricity.

Bio-Inspired Radiative Cooling Surfaces