Nuclear physics for multimessengers
APA
Caballero, L. (2018). Nuclear physics for multimessengers. Perimeter Institute. https://pirsa.org/18120024
MLA
Caballero, Lilianna. Nuclear physics for multimessengers. Perimeter Institute, Dec. 13, 2018, https://pirsa.org/18120024
BibTex
@misc{ pirsa_PIRSA:18120024, doi = {10.48660/18120024}, url = {https://pirsa.org/18120024}, author = {Caballero, Lilianna}, keywords = {Strong Gravity}, language = {en}, title = {Nuclear physics for multimessengers}, publisher = {Perimeter Institute}, year = {2018}, month = {dec}, note = {PIRSA:18120024 see, \url{https://pirsa.org}} }
Over the last few years gravitational wave (GW) detections have marked
the beginning of a new era of astrophysical observations. When the
emitters include a compact object like a neutron star, the GW signal
is accompanied by emissions in different bands, e.g. X-rays,
gamma-rays, optical and neutrinos. The interpretation of such
multimessenger signals allows us to gain a deeper understanding of the
interiors of compact objects. One main challenge is to link our
knowledge of nuclear interactions to macroscopic properties of dense
objects in the Universe. In this talk I will discuss selected aspects
along the interface of nuclear physics and astrophysics