Built on

E. Annala, T. Gorda, A. Kurkela, J. Nättilä, and A. Vuorinen, (2019), arXiv:1903.09121 [astro-ph.HE]
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1903
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T. Ishii, M. Järvinen, and G. Nijs, (2019), arXiv:1903.06169 [hep-ph]
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D. Pollney, C. Reisswig, L. Rezzolla, B. Szilágyi, M. Ansorg, B. Deris, P. Diener, E. N. Dorband, M. Koppitz, A. Nagar, and E. Schnetter, Phys. Rev. D 76
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W. H. Press, S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery, Numerical Recipes 3rd Edition: The Art of Scientific Computing , 3rd ed. (Cambridge University Press, New York, NY, USA, 2007)
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2019

Gravitational Waves from Holographic Neutron Star Mergers

Ecker, Christian, Järvinen, Matti, Nijs, Govert et al.

Understand

We simulate the merger of binary neutron stars and analyze the spectral properties of their gravitational waveforms.

For the stars we construct hybrid equations of state (EoSs) with a standard nuclear matter EoS at low densities, transitioning to a state-of-the-art holographic EoS in the otherwise intractable high density regime.
Depending on the transition density the characteristic frequencies in the spectrum produced from the hybrid EoSs are shifted to significantly lower values as compared to the pure nuclear matter EoS.
The highest rest-mass density reached outside a possible black hole horizon is approximately $1.1 \cdot 10^{15}$ g/cm$^3$, which for the holographic model is below the density of the deconfined quark matter phase.

Built on

E. Annala, T. Gorda, A. Kurkela, J. Nättilä, and A. Vuorinen, (2019), arXiv:1903.09121 [astro-ph.HE]
Original
1903
Earlier work this paper cites.
T. Ishii, M. Järvinen, and G. Nijs, (2019), arXiv:1903.06169 [hep-ph]
Original
1903
Earlier work this paper cites.
P. M. Chesler, N. Jokela, A. Loeb, and A. Vuorinen, (2019), arXiv:1906.08440 [astro-ph.HE]
Original
1906
Earlier work this paper cites.
S. Gandolfi, J. Carlson, and S. Reddy, Phys. Rev. C85
Original
1921
Earlier work this paper cites.
P. Haensel and B. Pichon, Astron. Astrophys. 283
1994
Earlier work this paper cites.
N. K. Glendenning, Compact stars: Nuclear physics, particle physics, and general relativity (1997)
1997
Earlier work this paper cites.
F. Banyuls, J. A. Font, J. M. Ibanez, J. M. Marti, and J. A. Miralles, The Astrophysical Journal 476
1997
Earlier work this paper cites.
F. Douchin and P. Haensel, Astron. Astrophys. 380
2001
Earlier work this paper cites.
E. Gourgoulhon, P. Grandclement, K. Taniguchi, J.-A. Marck, and S. Bonazzola, Phys. Rev. D63
2001
Earlier work this paper cites.
T. Goodale, G. Allen, G. Lanfermann, J. Massó, T. Radke, E. Seidel, and J. Shalf, in Vector and Parallel Processing – VECPAR’2002, 5th International Conference, Lecture Notes in Computer Science (Springer, Berlin, 2003)
2003
Earlier work this paper cites.
M. Alcubierre, B. Brügmann, P. Diener, M. Koppitz, D. Pollney, E. Seidel, and R. Takahashi, Phys. Rev. D 67
2003
Earlier work this paper cites.
E. Schnetter, S. H. Hawley, and I. Hawke, Class. Quant. Grav. 21
2004
Earlier work this paper cites.
J. Thornburg, Class. Quant. Grav. 21
2004
Earlier work this paper cites.
F. Bigazzi, R. Casero, A. L. Cotrone, E. Kiritsis, and A. Paredes, JHEP 10
2005
Earlier work this paper cites.
M. Alcubierre, Introduction to 3+1 Numerical Relativity (2006), 10.1093/acprof:oso/9780199205677.001.0001
2006
Earlier work this paper cites.
R. Casero, E. Kiritsis, and A. Paredes, Nucl. Phys. B787
2007
Earlier work this paper cites.
D. Pollney, C. Reisswig, L. Rezzolla, B. Szilágyi, M. Ansorg, B. Deris, P. Diener, E. N. Dorband, M. Koppitz, A. Nagar, and E. Schnetter, Phys. Rev. D 76
2007
Earlier work this paper cites.
W. H. Press, S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery, Numerical Recipes 3rd Edition: The Art of Scientific Computing , 3rd ed. (Cambridge University Press, New York, NY, USA, 2007)
2007
Earlier work this paper cites.

Similar

U. Gursoy and E. Kiritsis, JHEP 02
Original
2008
Cited alongside, same era.
M. Rozali, H.-H. Shieh, M. Van Raamsdonk, and J. Wu, JHEP 01
Original
2008
Cited alongside, same era.
U. Gursoy, E. Kiritsis, L. Mazzanti, and F. Nitti, Nucl. Phys. B820
Original
2009
Cited alongside, same era.
D. Brown, P. Diener, O. Sarbach, E. Schnetter, and M. Tiglio, Phys. Rev. D 79
2009
Cited alongside, same era.
A. Bauswein, H.-T. Janka, and R. Oechslin, Phys. Rev. D 82
2010
Cited alongside, same era.

Then

T. Alho, M. Järvinen, K. Kajantie, E. Kiritsis, C. Rosen, and K. Tuominen, JHEP 04
Original
2015
Later among the works it cites.
M. Järvinen, JHEP 07
Original
2015
Later among the works it cites.
S.-w. Li, A. Schmitt, and Q. Wang, Phys. Rev. D92
Original
2015
Later among the works it cites.
D. Radice, L. Rezzolla, and F. Galeazzi, Proceedings, Numerical Modeling of Space Plasma Flows (ASTRONUM-2014): Long Beach, CA, USA, June 23-27, 2014 , ASP Conf. Ser. 498
Original
2015
Later among the works it cites.
B. P. Abbott et al. (LIGO Scientific, Virgo), Phys. Rev. Lett. 116
Original

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

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M. Punturo et al. , Gravitational waves. Proceedings, 8th Edoardo Amaldi Conference, Amaldi 8, New York, USA, June 22-26, 2009 , Class. Quant. Grav. 27

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