TARDIS Papers and useful References

In the following a number of important works describing or using TARDIS are provided together with a collection of works outlining important techniques on which TARDIS is built.

TARDIS Code papers

Monte Carlo Radiative Transfer Works


[AbbottLucy85]D. C. Abbott and L. B. Lucy. Multiline transfer and the dynamics of stellar winds. Astrophysical Journal, 288:679–693, January 1985. doi:10.1086/162834.
[BarnaSzalaiKromer+17]B. Barna, T. Szalai, M. Kromer, W. E. Kerzendorf, J. Vinko, J. M. Silverman, G. H. Marion, and J. C. Wheeler. Abundance tomography of type iax sn 2011ay with tardis. ArXiv e-prints, July 2017. arXiv:1707.07848.
[BoyleSimHachingerKerzendorf17]A. Boyle, S. A. Sim, S. Hachinger, and W. Kerzendorf. Helium in double-detonation models of type ia supernovae. Astronomy and Astrophysics, 599:A46, March 2017. arXiv:1611.05938, doi:10.1051/0004-6361/201629712.
[CarterCashwell75]L. L. Carter and E. Cashwell. Particle-transport simulation with the Monte Carlo method. Technical Report, Los Alamos Scientific Laboratory, 1975. URL: http://www.iaea.org/inis/collection/NCLCollectionStore/_Public/07/227/7227109.pdf.
[HeringervanKerkwijkSimKerzendorf17]E. Heringer, M. H. van Kerkwijk, S. A. Sim, and W. E. Kerzendorf. Spectral sequences of Type Ia supernovae. I. Connecting normal and sub-luminous SN Ia and the presence of unburned carbon. ArXiv e-prints, July 2017. arXiv:1707.08572.
[InserraBullaSimSmartt16]C. Inserra, M. Bulla, S. A. Sim, and S. J. Smartt. Spectropolarimetry of superluminous supernovae: insight into their geometry. \apj , 831:79, November 2016. arXiv:1607.02353, doi:10.3847/0004-637X/831/1/79.
[KalosWhitlock08]M. H. Kalos and P. A. Whitlock. Monte Carlo Methods: Second Revised and Enlarged Edition. Wiley-VCH Verlag, 2008.
[KerzendorfSim14]W. E. Kerzendorf and S. A. Sim. A spectral synthesis code for rapid modelling of supernovae. Monthly Notices of the RAS, 440:387–404, May 2014. arXiv:1401.5469, doi:10.1093/mnras/stu055.
[LongKnigge02]K. S. Long and C. Knigge. Modeling the Spectral Signatures of Accretion Disk Winds: A New Monte Carlo Approach. Astrophysical Journal, 579:725–740, November 2002. arXiv:arXiv:astro-ph/0208011, doi:10.1086/342879.
[Lucy99a]L. B. Lucy. Computing radiative equilibria with Monte Carlo techniques. Astronomy and Astrophysics, 344:282–288, April 1999.
[Lucy99b]L. B. Lucy. Improved Monte Carlo techniques for the spectral synthesis of supernovae. Astronomy and Astrophysics, 345:211–220, May 1999.
[Lucy02]L. B. Lucy. Monte Carlo transition probabilities. Astronomy and Astrophysics, 384:725–735, March 2002. arXiv:arXiv:astro-ph/0107377, doi:10.1051/0004-6361:20011756.
[Lucy03]L. B. Lucy. Monte Carlo transition probabilities. II. Astronomy and Astrophysics, 403:261–275, May 2003. arXiv:arXiv:astro-ph/0303202, doi:10.1051/0004-6361:20030357.
[Lucy05]L. B. Lucy. Monte Carlo techniques for time-dependent radiative transfer in 3-D supernovae. Astronomy and Astrophysics, 429:19–30, January 2005. arXiv:arXiv:astro-ph/0409249, doi:10.1051/0004-6361:20041656.
[MageeKotakSim+16]M. R. Magee, R. Kotak, S. A. Sim, M. Kromer, D. Rabinowitz, S. J. Smartt, C. Baltay, H. C. Campbell, T.-W. Chen, M. Fink, A. Gal-Yam, L. Galbany, W. Hillebrandt, C. Inserra, E. Kankare, L. Le Guillou, J. D. Lyman, K. Maguire, R. Pakmor, F. K. Röpke, A. J. Ruiter, I. R. Seitenzahl, M. Sullivan, S. Valenti, and D. R. Young. The type Iax supernova, SN 2015H. A white dwarf deflagration candidate. Astronomy and Astrophysics, 589:A89, April 2016. arXiv:1603.04728, doi:10.1051/0004-6361/201528036.
[MageeKotakSim+17]M. R. Magee, R. Kotak, S. A. Sim, D. Wright, S. J. Smartt, E. Berger, R. Chornock, R. J. Foley, D. A. Howell, N. Kaiser, E. A. Magnier, R. Wainscoat, and C. Waters. Growing evidence that sne iax are not a one-parameter family. the case of ps1-12bwh. \aap , 601:A62, May 2017. arXiv:1701.05459, doi:10.1051/0004-6361/201629643.
[MazzaliLucy93]P. A. Mazzali and L. B. Lucy. The application of Monte Carlo methods to the synthesis of early-time supernovae spectra. Astronomy and Astrophysics, 279:447–456, November 1993.
[Noebauer14]U. M. Noebauer. A Monte Carlo Approach to Radiation Hydrodynamics in Stellar Outflows. PhD thesis, Technische Universität München, München, 2014. URL: http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:91-diss-20140731-1219398-0-8.
[SimProgaMiller+10]S. A. Sim, D. Proga, L. Miller, K. S. Long, and T. J. Turner. Multidimensional modelling of X-ray spectra for AGN accretion disc outflows - III. Application to a hydrodynamical simulation. Monthly Notices of the RAS, 408:1396–1408, November 2010. arXiv:1006.3449, doi:10.1111/j.1365-2966.2010.17215.x.