Probing Intermolecular Couplings in Simulations of the Two-Dimensional Infrared Photon Echo Spectrum of Liquid Water

Author(s):  
Alexander Paarmann ◽  
Tomoyuki Hayashi ◽  
Shaul Mukamel ◽  
R. J. Dwayne Miller
2008 ◽  
Vol 128 (19) ◽  
pp. 191103 ◽  
Author(s):  
A. Paarmann ◽  
T. Hayashi ◽  
S. Mukamel ◽  
R. J. D. Miller

Author(s):  
J. Stenger ◽  
D. Madsen ◽  
P. Hamm ◽  
E. T. J. Nibbering ◽  
T. Elsaesser

2004 ◽  
Vol 120 (21) ◽  
pp. 10215-10224 ◽  
Author(s):  
Prabuddha Mukherjee ◽  
Amber T. Krummel ◽  
Eric C. Fulmer ◽  
Itamar Kass ◽  
Isaiah T. Arkin ◽  
...  

Author(s):  
J. Stenger ◽  
D. Madsen ◽  
P. Hamm ◽  
E. T. J. Nibbering ◽  
T. Elsaesser

2020 ◽  
Vol 11 (1) ◽  
Author(s):  
Owen R. Lehmer ◽  
David C. Catling ◽  
Joshua Krissansen-Totton

AbstractIn the conventional habitable zone (HZ) concept, a CO2-H2O greenhouse maintains surface liquid water. Through the water-mediated carbonate-silicate weathering cycle, atmospheric CO2 partial pressure (pCO2) responds to changes in surface temperature, stabilizing the climate over geologic timescales. We show that this weathering feedback ought to produce a log-linear relationship between pCO2 and incident flux on Earth-like planets in the HZ. However, this trend has scatter because geophysical and physicochemical parameters can vary, such as land area for weathering and CO2 outgassing fluxes. Using a coupled climate and carbonate-silicate weathering model, we quantify the likely scatter in pCO2 with orbital distance throughout the HZ. From this dispersion, we predict a two-dimensional relationship between incident flux and pCO2 in the HZ and show that it could be detected from at least 83 (2σ) Earth-like exoplanet observations. If fewer Earth-like exoplanets are observed, testing the HZ hypothesis from this relationship could be difficult.


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