Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow

Kavli Affiliate: Yingjie Peng | First 5 Authors: Bocheng Zhu, Feng Yuan, Suoqing Ji, Yingjie Peng, Luis C. Ho | Summary: The cosmological inflow of a galaxy is speculated to be able to enter the galaxy and enhance the star formation rate (SFR) and black hole accretion rate (BHAR). In this paper, by performing high-resolution […]


Continue.. Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow

DESI survey validation data in the COSMOS/HSC field: Cool gas trace main sequence star-forming galaxies at the cosmic noon

Kavli Affiliate: Linhua Jiang | First 5 Authors: Siwei Zou, Linhua Jiang, Zheng Cai, John Moustakas, Zechang Sun | Summary: We present the first result in exploring the gaseous halo and galaxy correlation using the Dark Energy Spectroscopic Instrument (DESI) survey validation data in the Cosmic Evolution Survey (COSMOS) and Hyper Suprime-Cam (HSC) field. We […]


Continue.. DESI survey validation data in the COSMOS/HSC field: Cool gas trace main sequence star-forming galaxies at the cosmic noon

Quantum $z=2$ Lifshitz criticality in one-dimensional interacting fermions

Kavli Affiliate: Ke Wang | First 5 Authors: Ke Wang, , , , | Summary: We consider Lifshitz criticality (LC) with the dynamical critical exponent $z=2$ in one-dimensional interacting fermions with a filled Dirac Sea. We report that interactions have crucial effects on Lifshitz criticality. Single particle excitations are destabilized by interaction and decay into […]


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Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution

Sharon Lapiner, Avishai Dekel, Jonathan Freundlich, Omri Ginzburg, Fangzhou Jiang | Summary: [[{“value”:”We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend to undergo a robust `wet compaction’ event when near a `golden’ stellar mass of $sim 10^{10} M_{odot}$. This is a gaseous shrinkage to a compact star-forming phase, a `blue nugget’ (BN), followed […]


Continue.. Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution

Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution

Sharon Lapiner, Avishai Dekel, Jonathan Freundlich, Omri Ginzburg, Fangzhou Jiang | Summary: [[{“value”:”We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend to undergo a robust `wet compaction’ event when near a `golden’ stellar mass of $sim 10^{10} M_{odot}$. This is a gaseous shrinkage to a compact star-forming phase, a `blue nugget’ (BN), followed […]


Continue.. Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution

A novel fast response and radiation-resistant scintillator detector for beam loss monitor

Kavli Affiliate: Li Xin Li | First 5 Authors: Yuanjing Ji, Zebo Tang, Chen Li, Xin Li, Ming Shao | Summary: At high luminosity areas, beam loss monitor with fast response and high radiation resistance is crucial for accelerator operation. In this article, we report the design and test results of a fast response and […]


Continue.. A novel fast response and radiation-resistant scintillator detector for beam loss monitor

A novel fast response and radiation-resistant scintillator detector for beam loss monitor

Kavli Affiliate: Li Xin Li | First 5 Authors: Yuanjing Ji, Zebo Tang, Chen Li, Xin Li, Ming Shao | Summary: At high luminosity areas, beam loss monitor with fast response and high radiation resistance is crucial for accelerator operation. In this article, we report the design and test results of a fast response and […]


Continue.. A novel fast response and radiation-resistant scintillator detector for beam loss monitor

The Dark Side of Using Dark Sirens to Constrain the Hubble-LemaƮtre Constant

Kavli Affiliate: Xian Chen | First 5 Authors: Liang-Gui Zhu, Xian Chen, , , | Summary: Dark sirens, i.e., gravitational-wave (GW) sources without electromagnetic counterparts, are new probes of the expansion of the universe. The efficacy of this method relies on correctly localizing the host galaxies. However, recent theoretical studies have shown that astrophysical environments […]


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$g$-mode of neutron stars in pseudo-Newtonian gravity

Kavli Affiliate: Lijing Shao | First 5 Authors: Hong-Bo Li, Yong Gao, Lijing Shao, Renxin Xu, | Summary: The equation of state (EOS) of nuclear dense matter plays a crucial role in many astrophysical phenomena associated with neutron stars (NSs). Fluid oscillations are one of the most fundamental properties therein. NSs support a family of […]


Continue.. $g$-mode of neutron stars in pseudo-Newtonian gravity