Zobrazeno 1 - 10
of 415
pro vyhledávání: '"Storm, S."'
Autor:
Storm, S. David, Scherrer, Robert J.
We examine the power spectrum $P_n$ of the $n$th harmonic for Garfinkle-Vachaspati cosmic strings, which correspond to planar rectangular loops. While these loop tractories are self-intersecting, a slightly perturbed non-self-intersecting form of the
Externí odkaz:
http://arxiv.org/abs/2406.06743
Autor:
Storm, S. David, Scherrer, Robert J.
Publikováno v:
Phys. Lett. B, 829, 137126 (2022)
We examine the simplest inflection point quintessence model, with a potential given by $V(\phi) = V_0 + V_3 \phi^3$. This model can produce either asymptotic de Sitter expansion or transient acceleration, and we show that it does not correspond to ei
Externí odkaz:
http://arxiv.org/abs/2108.06378
Publikováno v:
In Radiography March 2024 30(2):582-588
Autor:
Brawley, Zachary T., Storm, S. David, Mora, Diego A. Contreras, Pelton, Matthew, Sheldon, Matthew
Vibrational strong coupling of molecules to optical cavities based on plasmonic resonances has been explored recently, because plasmonic near-fields can provide strong coupling in sub-diffraction limited volumes. Such field localization maximizes cou
Externí odkaz:
http://arxiv.org/abs/2012.00710
Autor:
Li, Chentao, Lu, Xin, Srivastava, Ajit, Storm, S. David, Gelfand, Rachel, Pelton, Matthew, Sukharev, Maxim, Harutyunyan, Hayk
Monolayer transition metal dichalcogenides, coupled to metal plasmonic nanocavities, have recently emerged as new platforms for strong light-matter interactions. These systems are expected to have nonlinear optical properties that will enable them to
Externí odkaz:
http://arxiv.org/abs/2009.08060
Autor:
Storm, S. David, Scherrer, Robert J.
Publikováno v:
Phys. Rev. D 102, 063519 (2020)
We examine the Swampland conjectures in the context of generic slow-roll thawing quintessence models. Defining $\lambda \equiv |V^{\prime}(\phi_i)/V(\phi_i)|$ and $K \equiv \sqrt{1 - 4V^{\prime \prime}(\phi_i)/3V(\phi_i)}$, where $\phi_i$ is the init
Externí odkaz:
http://arxiv.org/abs/2008.05465
Autor:
Guidi, G., Tazzari, M., Testi, L., de Gregorio-Monsalvo, I., Chandler, C. J., Pérez, L., Isella, A., Natta, A., Ortolani, S., Hennings, Th., Corder, S., Linz, H., Andrews, S., Wilner, D., Ricci, L., Carpenter, J., Sargent, A., Mundy, L., Storm, S., Calvet, N., Dullemond, C., Greaves, J., Lazio, J., Deller, A., Kwon, W.
Publikováno v:
A&A 588, A112 (2016)
To characterize the mechanisms of planet formation it is crucial to investigate the properties and evolution of protoplanetary disks around young stars, where the initial conditions for the growth of planets are set. Our goal is to study grain growth
Externí odkaz:
http://arxiv.org/abs/1601.07542
Autor:
Tazzari, M., Testi, L., Ercolano, B., Natta, A., Isella, A., Chandler, C. J., Pérez, L. M., Andrews, S., Wilner, D. J., Ricci, L., Henning, T., Linz, H., Kwon, W., Corder, S. A., Dullemond, C. P., Carpenter, J. M., Sargent, A. I., Mundy, L., Storm, S., Calvet, N., Greaves, J. A., Lazio, J., Deller, A. T.
Publikováno v:
A&A 588, A53 (2016)
Theoretical models of grain growth predict dust properties to change as a function of protoplanetary disk radius, mass, age and other physical conditions. We lay down the methodology for a multi-wavelength analysis of (sub-)mm and cm continuum interf
Externí odkaz:
http://arxiv.org/abs/1512.05679
Autor:
Storm, S., Mundy, L. G., Fernández-López, M., Lee, K. I., Looney, L. W., Teuben, P. J., Rosolowsky, E., Arce, H. G., Ostriker, E. C., Segura-Cox, D., Pound, M. W., Salter, D. M., Volgenau, N. H., Shirley, Y. L., Chen, C., Gong, H., Plunkett, A. L., Tobin, J. J., Kwon, W., Isella, A., Kauffmann, J., Tassis, K., Crutcher, R. M., Gammie, C. F., Testi, L.
We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N2H+, HCO+, and HCN (J=1-0 transitions) across over 800 square arcminutes of
Externí odkaz:
http://arxiv.org/abs/1409.1233
Autor:
Fernández-López, M., Arce, H. G., Looney, L., Mundy, L. G., Storm, S., Teuben, P. J., Lee, K., Segura-Cox, D., Isella, A., Tobin, J. J., Rosolowsky, E., Plunkett, A., Kwon, W., Kauffmann, J., Ostriker, E., Tassis, K., Shirley, Y. L., Pound, M.
Publikováno v:
2014, ApJ, 790, L19
We present the N2H+(J=1-0) map of the Serpens South molecular cloud obtained as part of the CARMA Large Area Star Formation Survey (CLASSy). The observations cover 250 square arcminutes and fully sample structures from 3000 AU to 3 pc with a velocity
Externí odkaz:
http://arxiv.org/abs/1407.0755