Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Shingles, L. J."'
Autor:
Callan, F. P., Collins, C. E., Sim, S. A., Shingles, L. J., Pakmor, R., Srivastav, S., Pollin, J. M., Gronow, S., Roepke, F. K., Seitenzahl, I. R.
In the double detonation scenario the ignition of a surface He detonation on a sub-Chandrasekhar mass white dwarf leads to a secondary core detonation. Double detonation models have shown promise for explaining Type Ia supernovae (SNe Ia) with a vari
Externí odkaz:
http://arxiv.org/abs/2408.03048
Autor:
Pollin, J. M., Sim, S. A., Pakmor, R., Callan, F. P., Collins, C. E., Shingles, L. J., Roepke, F. K., Srivastav, S.
A leading model for Type Ia supernovae involves the double-detonation of a sub-Chandrasekhar mass white dwarf. Double-detonations arise when a surface helium shell detonation generates shockwaves that trigger a core detonation; this mechanism may be
Externí odkaz:
http://arxiv.org/abs/2408.00917
Autor:
Callan, F. P., Sim, S. A., Collins, C. E., Shingles, L. J., Lach, F., Roepke, F. K., Pakmor, R., Kromer, M., Srivastav, S.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 530, Issue 2, May 2024, Pages 1457 to 1473
Type Iax supernovae (SNe Iax) are proposed to arise from deflagrations of Chandrasekhar mass white dwarfs (WDs). Previous deflagration simulations have achieved good agreement with the light curves and spectra of intermediate-luminosity and bright SN
Externí odkaz:
http://arxiv.org/abs/2403.15084
Autor:
Shingles, L. J., Sim, S. A., Kromer, M., Maguire, K., Bulla, M., Collins, C., Ballance, C. P., Michel, A. S., Ramsbottom, C. A., Roepke, F. K., Seitenzahl, I. R., Tyndall, N. B.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 492, Issue 2, February 2020, Pages 2029-2043
We extend the range of validity of the ARTIS 3D radiative transfer code up to hundreds of days after explosion, when Type Ia supernovae are in their nebular phase. To achieve this, we add a non-local thermodynamic equilibrium (non-LTE) population and
Externí odkaz:
http://arxiv.org/abs/1912.02214
Autor:
Smartt, S. J., Chen, T. -W., Jerkstrand, A., Coughlin, M., Kankare, E., Sim, S. A., Fraser, M., Inserra, C., Maguire, K., Chambers, K. C., Huber, M. E., Kruhler, T., Leloudas, G., Magee, M., Shingles, L. J., Smith, K. W., Young, D. R., Tonry, J., Kotak, R., Gal-Yam, A., Lyman, J. D., Homan, D. S., Agliozzo, C., Anderson, J. P., Ashall, C. R. Angus C., Barbarino, C., Bauer, F. E., Berton, M., Botticella, M. T., Bulla, M., Bulger, J., Cannizzaro, G., Cano, Z., Cartier, R., Cikota, A., Clark, P., De Cia, A., Della Valle, M., Denneau, L., Dennefeld, M., Dessart, L., Dimitriadis, G., Elias-Rosa, N., Firth, R. E., Flewelling, H., Flors, A., Franckowiak, A., Frohmaier, C., Galbany, L., Gonzalez-Gaitan, S., Greiner, J., Gromadzki, M., Guelbenzu, A. Nicuesa, Gutierrez, C. P., Hamanowicz, A., Hanlon, L., Harmanen, J., Heintz, K. E., Heinze, A., Hernandez, M. -S., Hodgkin, S. T., Hook, I. M., Izzo, L., James, P. A., Jonker, P. G., Kerzendorf, W. E., Klose, S., Kostrzewa-Rutkowska, Z., Kowalski, M., Kromer, M., Kuncarayakti, H., Lawrence, A., Lowe, T. B., Magnier, E. A., Manulis, I., Martin-Carrillo, A., Mattila, S., McBrien, O., Muller, A., Nordin, J., O'Neill, D., Onori, F., Palmerio, J. T., Pastorello, A., Patat, F., Pignata, G., Podsiadlowski, Ph., Pumo, M. L., Prentice, S. J., Rau, A., Razza, A., Rest, A., Reynolds, T., Roy, R., Ruiter, A. J., Rybicki, K. A., Salmon, L., Schady, P., Schultz, A. S. B., Schweyer, T., Seitenzahl, I. R., Smith, M., Sollerman, J., Stalder, B., Stubbs, C. W., Sullivan, M., Szegedi, H., Taddia, F., Taubenberger, S., Terreran, G., van Soelen, B., Vos, J., Wainscoat, R. J., Walton, N. A., Waters, C., Weiland, H., Willman, M., Wiseman, P., Wright, D. E., Wyrzykowski, L., Yaron, O.
Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to eject material rich in heavy radioactive isotopes that can power an el
Externí odkaz:
http://arxiv.org/abs/1710.05841
Autor:
Pollin, J M, Sim, S A, Pakmor, R, Callan, F P, Collins, C E, Shingles, L J, Röpke, F K, Srivastav, S
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 9/30/2024, Vol. 533 Issue 3, p3036-3052, 17p
Autor:
Callan, F P, Sim, S A, Collins, C E, Shingles, L J, Lach, F, Röpke, F K, Pakmor, R, Kromer, M, Srivastav, S
Publikováno v:
Monthly Notices of the Royal Astronomical Society; May2024, Vol. 530 Issue 2, p1457-1473, 17p
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Autor:
Flörs, A., Silva, R. F., Deprince, J., Gallego, H. Carvajal, Leck, G., Shingles, L. J., Martínez-Pinedo, G., Sampaio, J. M., Amaro, P., Marques, J. P., Goriely, S., Quinet, P., Palmeri, P., Godefroid, M.
ACKNOWLEDGEMENTS AF, GL, LJS and GMP acknowledge support by the European Research Council (ERC) under the State of Hesse within the Cluster Project ELEMENTS. JD and SG acknowledge financial support from F.R.S.-FNRS (Belgium). RFS, JMS, JPM and PA ack
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1437::ada5b5f28a47c252c7a5b2ef1cb455c5
https://hdl.handle.net/10362/155553
https://hdl.handle.net/10362/155553
Autor:
Flörs, A, Silva, R F, Deprince, J, Carvajal Gallego, H, Leck, G, Shingles, L J, Martínez-Pinedo, G, Sampaio, J M, Amaro, P, Marques, J P, Goriely, S, Quinet, P, Palmeri, P, Godefroid, M
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Sep2023, Vol. 524 Issue 2, p3083-3101, 19p