Short-range correlations soften neutron-star equations of state with quadratic vector self-interactions but stiffen them with an added fourth-order term, producing corresponding shifts in maximum masses that persist when a dark-matter fluid is included.
SKA-Athena Synergy White Paper
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
abstract
The Advanced Telescope for High Energy Astrophysics (Athena) is the X-ray observatory large mission selected by the European Space Agency (ESA), within its Cosmic Vision 2015-2025 programme, to address the "Hot and Energetic Universe" scientific theme (Nandra et al. 2013), and it is provisionally due for launch in the early 2030s. The Square Kilometer Array (SKA) is the next generation radio observatory and consists of two telescopes, one comprised of dishes operating at mid frequencies (SKA1-MID) and located in South Africa, and the other comprised of Log-Periodic antennas operating at low radio frequencies (SKA1-LOW), which will be located in Australia (Braun et al. 2017). The scientific commissioning of the radio telescope is planned to begin in 2021-2022. The SKA-Athena Synergy Team (SAST) has been tasked to single out the potential scientific synergies between Athena and SKA. The astrophysical community was involved in this exercise primarily through a dedicated SKA-Athena Synergy Workshop, which took place on April 24-25, 2017 at SKAO, Jodrell Bank, Manchester. The final result of the synergy exercise, this White Paper, describes in detail a number of scientific opportunities that will be opened up by the combination of Athena and SKA, these include: 1. the Cosmic Dawn; 2. the Evolution of black holes and galaxies; 3. Active galaxy feedback in galaxy clusters; 4. Non-thermal phenomena in galaxy clusters; 5. Detecting the cosmic web; 6. Black-hole accretion physics and astrophysical transients; 7. Galactic astronomy: stars, planets, pulsars and supernovae.
verdicts
UNVERDICTED 2representative citing papers
A literature review finds that a high fraction of low-mass galaxies host intermediate-mass black holes below 100,000 solar masses, with no solid detections in globular clusters and the black hole mass-stellar velocity dispersion relation extending unbroken to lower masses despite large scatter.
citing papers explorer
-
Effects of short-range correlations at high densities on neutron stars with and without DM content: role of the repulsive self-interaction
Short-range correlations soften neutron-star equations of state with quadratic vector self-interactions but stiffen them with an added fourth-order term, producing corresponding shifts in maximum masses that persist when a dark-matter fluid is included.
-
Intermediate-Mass Black Holes
A literature review finds that a high fraction of low-mass galaxies host intermediate-mass black holes below 100,000 solar masses, with no solid detections in globular clusters and the black hole mass-stellar velocity dispersion relation extending unbroken to lower masses despite large scatter.