Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Robert P. Harkness"'
Autor:
Arun Parupudi, Sumit K. Chaturvedi, Regina Adão, Robert W. Harkness, Sonia Dragulin-Otto, Lewis E. Kay, Reza Esfandiary, Huaying Zhao, Peter Schuck
Publikováno v:
Scientific Reports, Vol 11, Iss 1, Pp 1-15 (2021)
Abstract Weak macromolecular interactions assume a dominant role in the behavior of highly concentrated solutions, and are at the center of a variety of fields ranging from colloidal chemistry to cell biology, neurodegenerative diseases, and manufact
Externí odkaz:
https://doaj.org/article/e909457b3b7a460aaae039df639e78fb
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-10 (2018)
Complex assembly pathways often involve transient, partly-formed intermediates that are challenging to characterize. Here, the authors present a simple and rapid spectroscopic thermal hysteresis method for mapping the energy landscapes of supramolecu
Externí odkaz:
https://doaj.org/article/69a96f65f7364d2ebdc35ca9920a4ee7
Autor:
Brian W. O'Shea, Robert P. Harkness, Michael L. Norman, Jack O. Burns, Rick Wagner, Eric J. Hallman
Publikováno v:
The Astrophysical Journal. 671:27-39
We present the first results from a new generation of simulated large sky coverage (~100 square degrees) Sunyaev-Zeldovich effect (SZE) cluster surveys using the cosmological adaptive mesh refinement N-body/hydro code Enzo. We have simulated a very l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::982e9c9809e7821ab976c3d2c984957a
https://doi.org/10.1086/522912
https://doi.org/10.1086/522912
Publikováno v:
The Astrophysical Journal. 496:908-914
Models of infrared spectra of Type Ia supernovae around maximum light are presented. The underlying dynamic models are delayed detonation explosions in Chandrasekhar mass carbon/oxygen white dwarfs. In combination with the radiative transport codes e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ab65276636f37e29b773227efa3467d2
https://doi.org/10.1086/305427
https://doi.org/10.1086/305427
Autor:
Andrew C. Phillips, A. Clocchiatti, M. R. Rosa, John C Wheeler, P. O. Lindblad, N. B. Suntzeff, Robert P. Harkness, Alexei V. Filippenko, M. M. Phillips, Stefano Cristiani, K. Beuermann, P. Grosbøl, Michael A. Dopita
Publikováno v:
The Astrophysical Journal. 483:675-697
We present CCD photometry and low-resolution spectra of the spectroscopic Type Ic supernova SN 1983V in NGC 1365. Photometry in the B band spans nearly 250 days after maximum light, while the spectra cover the photospheric epoch, from 9 days before u
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3c752d1128bfff9d9aca7d2fc262ac6c
https://doi.org/10.1086/304268
https://doi.org/10.1086/304268
Publikováno v:
Physics Reports. 256:211-235
We argue here that models of SN Ia based on gravitational collapse with the ejection of only a small amount of matter and nickel will be subluminous, and are likely to have problems with the light curve and especially with the spectral evolution. Can
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b66652e147c55b7f93aeb4bc5c866467
https://doi.org/10.1016/0370-1573(94)00109-g
https://doi.org/10.1016/0370-1573(94)00109-g
Autor:
Michael E. Papka, Rick Wagner, Mark Hereld, Robert P. Harkness, Daniel R. Reynolds, Michael L. Norman, Joseph A. Insley
Publikováno v:
SC Companion
The light from early galaxies had a dramatic impact on the gasses filling the universe. This video highlights the spatial structure of the light's effect, by comparing two simulations: one with a self-consistent radiation field (radiative), and one w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fb993eb21d8f6655902d3232fea6ee1d
https://doi.org/10.1109/sc.companion.2012.329
https://doi.org/10.1109/sc.companion.2012.329
Autor:
Dan Reynolds, Michael L. Norman, Manisha Gajbe, Michael Kuhlen, John H. Wise, Dave Semeraro, Mathew Turk, Brian W. O'Shea, Robert P. Harkness, Britton D. Smith
Publikováno v:
SC Companion
The submitted visualization represents work performed by the Enzo PRAC team lead by Brian O'Shea on the Blue Waters Early Science system. A relatively small test calculation was performed followed by several much larger AMR cosmological runs. The ove
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::56ec3ac1a57fa9cf9a506abe81267c58
https://doi.org/10.1109/sc.companion.2012.370
https://doi.org/10.1109/sc.companion.2012.370
Autor:
Daniel R. Reynolds, Michael E. Papka, Joseph A. Insley, Mark Hereld, Michael L. Norman, Rick Wagner, Robert P. Harkness
Publikováno v:
SC Companion
The light from early galaxies had a dramatic impact on the gasses filling the universe. This video highlights the spatial structure of the light's effect, by comparing two simulations: one with a self-consistent radiation field (radiative), and one w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::accc26bbfc592bc8c86a1aa084b8b74f
https://doi.org/10.1109/sc.companion.2012.328
https://doi.org/10.1109/sc.companion.2012.328
Autor:
Rick Wagner, Michael E. Papka, Robert P. Harkness, Daniel R. Reynolds, Venkatram Vishwanath, Eric C. Olson, Michael L. Norman, Joseph A. Insley, Mark Hereld
Publikováno v:
SC Companion
This simulation uses a flux-limited diffusion solver to explore the radiation hydrodynamics of early galaxies, in particular, the ionizing radiation created by Population III stars. At the time of this rendering, the simulation has evolved to a redsh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f4088140ea4292f8b4bef54b58f6fecd
https://doi.org/10.1145/2148600.2148674
https://doi.org/10.1145/2148600.2148674