Explore the words cloud of the Burst3D project. It provides you a very rough idea of what is the project "Burst3D" about.
The following table provides information about the project.
UNIVERSITY OF SOUTHAMPTON
|Coordinator Country||United Kingdom [UK]|
|Total cost||251˙857 €|
|EC max contribution||251˙857 € (100%)|
1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
|Duration (year-month-day)||from 2016-10-01 to 2019-09-30|
Take a look of project's partnership.
|1||UNIVERSITY OF SOUTHAMPTON||UK (SOUTHAMPTON)||coordinator||251˙857.00|
|2||TRUSTEES OF PRINCETON UNIVERSITY||US (PRINCETON, NJ)||partner||0.00|
On Earth, nuclear explosions take place in controlled environments or use small amounts of fuel. Despite that, they generate spectacular amounts of energy. When nuclear reactions ignite on a neutron star, the whole surface can burn, resulting in extremely bright X-ray flashes that outshine all the other emission. These flashes are known as type I bursts. Their emission encodes information about the neutron star mass and radius and this makes them ideal probes to explore such stars' properties. Much effort has been invested to describe nuclear explosions, both on Earth and in space, but the modelling of the type I bursts entails extra difficulties. In particular, simulating deflagrating flames in the extreme conditions of neutron stars has proven particularly challenging. Nonetheless, in the last several years I have been able to produce the first ab initio 2D simulations of type I bursts where the deflagration takes place inside a burning hurricane that expands to engulf the whole surface of the star. However, 2D simulations have inherent limitations. With this project I intend to model the nuclear explosions during the bursts combining detailed microphysics with a magnetohydrodynamical description set for the first time in a 3D spherical geometry to be able to capture the combination of all the relevant effects. Understanding all the different facets of the bursts and their physical ingredients, I will produce unprecedented simulations which I will couple to a ray tracing code that takes into account the general relativistic effects of the star's gravity and rotation on the emitted photons. I will be able to produce extremely accurate synthetic lightcurves to confront with the observations in order to extract the information about the neutron star contained in the X-ray emission. Once the parameters of the bursters are known, these can be used to constrain the yet unknown behavior of matter in the core of neutron stars.
|year||authors and title||journal||last update|
Ray, Paul S.; Arzoumanian, Zaven; Ballantyne, David; Bozzo, Enrico; Brandt, Soren; Brenneman, Laura; Chakrabarty, Deepto; Christophersen, Marc; DeRosa, Alessandra; Feroci, Marco; Gendreau, Keith; Goldstein, Adam; Hartmann, Dieter; Hernanz, Margarita; Jenke, Peter; Kara, Erin; Maccarone, Tom; McDonald, Michael; Nowak, Michael; Phlips, Bernard Remillard, Ron; Stevens, Abigail; Tomsick, John; Watts,
STROBE-X: X-ray Timing and Spectroscopy on Dynamical Timescales from Microseconds to Years
published pages: , ISSN: , DOI:
Jean J. M. in â€™t Zand, Enrico Bozzo, JinLu Qu, Xiang-Dong Li, Lorenzo Amati, Yang Chen, Immacolata Donnarumma, Victor Doroshenko, Stephen A. Drake, Margarita Hernanz, Peter A. Jenke, Thomas J. Maccarone, Simin Mahmoodifar, Domitilla de Martino, Alessandra De Rosa, Elena M. Rossi, Antonia Rowlinson, Gloria Sala, Giulia Stratta, Thomas M. Tauris, Joern Wilms, XueFeng Wu, Ping Zhou, IvÃ¡n Agudo, Di
Observatory science with eXTP
published pages: , ISSN: 1674-7348, DOI: 10.1007/s11433-017-9186-1
|Science China Physics, Mechanics & Astronomy 62/2||2020-01-29|
Anna L. Watts, WenFei Yu, Juri Poutanen, Shu Zhang, Sudip Bhattacharyya, Slavko Bogdanov, Long Ji, Alessandro Patruno, Thomas E. Riley, Pavel Bakala, Altan Baykal, Federico Bernardini, Ignazio Bombaci, Edward Brown, Yuri Cavecchi, Deepto Chakrabarty, JÃ©rÃ´me Chenevez, Nathalie Degenaar, Melania Del Santo, Tiziana Di Salvo, Victor Doroshenko, Maurizio Falanga, Robert D. Ferdman, Marco Feroci, Ange
Dense matter with eXTP
published pages: , ISSN: 1674-7348, DOI: 10.1007/s11433-017-9188-4
|Science China Physics, Mechanics & Astronomy 62/2||2020-01-29|
Yuri Cavecchi, Anatoly Spitkovsky
Three-dimensional Instability of Flame Fronts in Type I X-Ray Bursts
published pages: 142, ISSN: 1538-4357, DOI: 10.3847/1538-4357/ab3650
|The Astrophysical Journal 882/2||2020-01-29|
M. Zingale, K. Eiden, Y. Cavecchi, A. Harpole, J. B. Bell, M. Chang, I. Hawke, M. P. Katz, C. M. Malone, A. J. Nonaka, D. E. Willcox, W. Zhang
Toward Resolved Simulations of Burning Fronts in Thermonuclear X-ray Bursts
published pages: 12005, ISSN: 1742-6588, DOI: 10.1088/1742-6596/1225/1/012005
|Journal of Physics: Conference Series 1225||2020-01-29|
Frank R. N. Chambers, Anna L. Watts, Laurens Keek, Yuri Cavecchi, Ferran Garcia
Burning in the Tail: Implications for a Burst Oscillation Model
published pages: 61, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aaf501
|The Astrophysical Journal 871/1||2020-01-29|
C. Ceccobello, Y. Cavecchi, M. H. M. Heemskerk, S. Markoff, P. Polko, D. Meier
A new method for extending solutions to the self-similar relativistic magnetohydrodynamic equations for black hole outflows
published pages: 4417-4435, ISSN: 0035-8711, DOI: 10.1093/mnras/stx2567
|Monthly Notices of the Royal Astronomical Society 473/4||2020-01-29|
Yuri Cavecchi, Anna L. Watts, Duncan K. Galloway
On the Dependence of the X-Ray Burst Rate on Accretion and Spin Rate
published pages: 1, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aa9897
|The Astrophysical Journal 851/1||2020-01-29|
F R N Chambers, A L Watts, Y Cavecchi, F Garcia, L Keek
Superburst oscillations: ocean and crustal modes excited by carbon-triggered type I X-ray bursts
published pages: 4391-4402, ISSN: 0035-8711, DOI: 10.1093/mnras/sty895
|Monthly Notices of the Royal Astronomical Society 477/4||2020-01-29|
L E RiveraÂ Sandoval, R Wijnands, N Degenaar, Y Cavecchi, C O Heinke, E M Cackett, J Homan, D Altamirano, A Bahramian, G R Sivakoff, J M Miller, A S Parikh
Extreme quiescent variability of the transient neutron star low-mass X-ray binary EXO 1745âˆ’248 in Terzan 5
published pages: 2777-2788, ISSN: 0035-8711, DOI: 10.1093/mnras/sty1535
|Monthly Notices of the Royal Astronomical Society 479/2||2020-01-29|
Patrick Crumley, Chiara Ceccobello, Riley M. T. Connors, Yuri Cavecchi
The jet-disk symbiosis without maximal jets : 1D hydrodynamical jets revisited
published pages: A87, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201630229
|Astronomy & Astrophysics 601||2020-01-29|
A. Rouco Escorial, A. S. Bak Nielsen, R. Wijnands, Y. Cavecchi, N. Degenaar, A. Patruno
The low-luminosity behaviour of the 4U 0115+63 Be/X-ray transient
published pages: 1802-1808, ISSN: 0035-8711, DOI: 10.1093/mnras/stx2111
|Monthly Notices of the Royal Astronomical Society 472/2||2020-01-29|
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