Tristan L. Smith, Ph.D.
Affiliations: | 2008 | Physics | California Institute of Technology, Pasadena, CA |
Area:
Cosmology, particle astrophysics, astrophysics, particle physicsGoogle:
"Tristan Smith"Mean distance: 15.11 | S | N | B | C | P |
Parents
Sign in to add mentor| Marc P. Kamionkowski | grad student | 2008 | Caltech | |
| (The gravity of the situation.) | ||||
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Publications
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| Smith TL, Poulin V, Amin MA. (2020) Oscillating scalar fields and the Hubble tension: A resolution with novel signatures Physical Review D. 101 |
| Cookmeyer J, Grin D, Smith TL. (2020) How sound are our ultralight axion approximations? Physical Review D. 101 |
| Poulin V, Smith TL, Karwal T, et al. (2019) Early Dark Energy can Resolve the Hubble Tension. Physical Review Letters. 122: 221301 |
| Smith TL, Grin D, Robinson D, et al. (2019) Probing spatial variation of the fine-structure constant using the CMB Physical Review D. 99 |
| Smith TL, Caldwell RR. (2019) LISA for cosmologists: Calculating the signal-to-noise ratio for stochastic and deterministic sources Physical Review D. 100 |
| Hazboun JS, Romano JD, Smith TL. (2019) Realistic sensitivity curves for pulsar timing arrays Physical Review D. 100 |
| Burke-Spolaor S, Taylor SR, Charisi M, et al. (2019) The astrophysics of nanohertz gravitational waves The Astronomy and Astrophysics Review. 27 |
| Poulin V, Smith TL, Grin D, et al. (2018) Cosmological implications of ultralight axionlike fields Physical Review D. 98 |
| Smith TL, Muñoz JB, Smith R, et al. (2017) Baryons still trace dark matter: Probing CMB lensing maps for hidden isocurvature Physical Review D. 96 |
| Smith TL, Caldwell R. (2017) Sensitivity to a frequency-dependent circular polarization in an isotropic stochastic gravitational wave background Physical Review D. 95 |