@article{https://doi.org/10.48550/arxiv.2105.00798,<br/><span class="tab"></span>
  doi = {10.48550/ARXIV.2105.00798},<br/><span class="tab"></span>
  url = {https://arxiv.org/abs/2105.00798},<br/><span class="tab"></span>
  author = {Yeung,<br/><span class="tab"></span> Cheung-Hei and Lin,<br/><span class="tab"></span> Lap-Ming and Andersson,<br/><span class="tab"></span> Nils and Comer,<br/><span class="tab"></span> Greg},<br/><span class="tab"></span>
  keywords = {High Energy Astrophysical Phenomena (astro-ph.HE),<br/><span class="tab"></span> Solar and Stellar Astrophysics (astro-ph.SR),<br/><span class="tab"></span> General Relativity and Quantum Cosmology (gr-qc),<br/><span class="tab"></span> Nuclear Theory (nucl-th),<br/><span class="tab"></span> FOS: Physical sciences,<br/><span class="tab"></span> FOS: Physical sciences},<br/><span class="tab"></span>
  title = {The I-Love-Q Relations for Superfluid Neutron Stars},<br/><span class="tab"></span>
  publisher = {arXiv},<br/><span class="tab"></span>
  year = {2021},<br/><span class="tab"></span>
  copyright = {Creative Commons Attribution 4.0 International}
}