collaborators

6 papers

cond-mat.soft2026

Density-Selected Topological Pathways in the Melting of Single-Particle-Thick Stripes

José Rafael Bordin

The melting of stripe-forming systems involves changes in connectivity that are not fully captured by conventional structural and orientational descriptors. We investigate a two-di…

astro-ph.IM2026

Detecting habitable exoplanet atmospheres with LIFE, the Large Interferometer for Exoplanets

Sarah Rugheimer, Aiden Weatherbee, James Fecanin +21

A key goal of astronomers with the next generation telescopes is to detect signs of life in exoplanet atmospheres. NASA's next flagship is the Habitable Worlds Observatory (HWO). I…

astro-ph.EP2026

Organosulfur Chemistry on sub-Neptunes: Implications for hazes and biosignatures

Sean Jordan, Shang-Min Tsai, Paul B. Rimmer +1

The organosulfur biosignature gases dimethylsulfide (DMS) and dimethlydisulfide (DMDS) have recently been claimed to be present in the atmosphere of sub-Neptune exoplanet K2-18b, l…

astro-ph.EP2026

Comparative biosignatures with systemic retrievals

Tereza Constantinou, Oliver Shorttle, Miles Cranmer +1

The discovery of inhabited exoplanets hinges on identifying biosignature gases. JWST can reveal biosignature gases, though current discoveries have yet to evidence life. The centra…

astro-ph.EP2025

Powerful lightning on Venus constrained by atmospheric NO

Tereza Constantinou, Oliver Shorttle, Paul B. Rimmer

Signs of lightning on Venus have long been sought, including by space missions and ground-based telescopes searching for optical flashes, plasma waves, or radio signatures. These e…

astro-ph.EP2025

Abiotic Ozone in the Observable Atmospheres of Venus and Venus-like Exoplanets

Robb Calder, Oliver Shorttle, Sean Jordan +2

Ozone is a potential biosignature and disambuguator between Earth-like and Venus-like exoplanets due to its association on Earth with photosynthetically produced oxygen (O). Ho…