Steering-induced phase transition in measurement-only quantum circuits

Kavli Affiliate: Jing Wang | First 5 Authors: Dongheng Qian, Jing Wang, , , | Summary: Competing measurements alone can give rise to distinct phases characterized by entanglement entropy$unicode{x2013}$such as the volume law phase, symmetry-breaking (SB) phase, and symmetry-protected topological (SPT) phase$unicode{x2013}$that can only be discerned through quantum trajectories, making them challenging to observe experimentally. […]


Continue.. Steering-induced phase transition in measurement-only quantum circuits

Steering-induced phase transition in measurement-only quantum circuits

Kavli Affiliate: Jing Wang | First 5 Authors: Dongheng Qian, Jing Wang, , , | Summary: Competing measurements alone can give rise to distinct phases characterized by entanglement entropy$unicode{x2013}$such as the volume law phase, symmetry-breaking (SB) phase, and symmetry-protected topological (SPT) phase$unicode{x2013}$that can only be discerned through quantum trajectories, making them challenging to observe experimentally. […]


Continue.. Steering-induced phase transition in measurement-only quantum circuits

Characterize the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias

Kavli Affiliate: Yingjie Peng | First 5 Authors: Kai Wang, H. J. Mo, Yangyao Chen, Huiyuan Wang, Xiaohu Yang | Summary: We propose a novel method to quantify the assembly histories of dark matter halos with the redshift evolution of the mass-weighted spatial variance of their progenitor halos, i.e. the protohalo size history. We find […]


Continue.. Characterize the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias

Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias

Kavli Affiliate: Yingjie Peng | First 5 Authors: Kai Wang, H. J. Mo, Yangyao Chen, Huiyuan Wang, Xiaohu Yang | Summary: We propose a novel method to quantify the assembly histories of dark matter halos with the redshift evolution of the mass-weighted spatial variance of their progenitor halos, i.e. the protohalo size history. We find […]


Continue.. Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias

A large population of strongly lensed faint submillimetre galaxies in future dark energy surveys inferred from JWST imaging

Kavli Affiliate: Luis C. Ho | First 5 Authors: James Pearson, Stephen Serjeant, Wei-Hao Wang, Zhen-Kai Gao, Arif Babul | Summary: Bright galaxies at sub-millimetre wavelengths from Herschel are now well known to be predominantly strongly gravitationally lensed. The same models that successfully predicted this strongly lensed population also predict about one percent of faint […]


Continue.. A large population of strongly lensed faint submillimetre galaxies in future dark energy surveys inferred from JWST imaging

A large population of strongly lensed faint submillimetre galaxies in future dark energy surveys inferred from JWST imaging

Kavli Affiliate: Luis C. Ho | First 5 Authors: James Pearson, Stephen Serjeant, Wei-Hao Wang, Zhen-Kai Gao, Arif Babul | Summary: Bright galaxies at sub-millimetre wavelengths from Herschel are now well known to be predominantly strongly gravitationally lensed. The same models that successfully predicted this strongly lensed population also predict about one percent of faint […]


Continue.. A large population of strongly lensed faint submillimetre galaxies in future dark energy surveys inferred from JWST imaging

VLBI Observations of a sample of Palomar-Green quasars II: characterising the parsec-scale radio emission

Kavli Affiliate: Luis C. Ho | First 5 Authors: Ailing Wang, Tao An, Yingkang Zhang, Xiaopeng Cheng, Luis C. Ho | Summary: This study uses multi-frequency Very Long Baseline Interferometry (VLBI) to study the radio emission from 10 radio-quiet quasars (RQQs) and four radio-loud quasars (RLQs). The diverse morphologies, radio spectra, and brightness temperatures observed […]


Continue.. VLBI Observations of a sample of Palomar-Green quasars II: characterising the parsec-scale radio emission

UV-Optical Emission of AB Aur b is Consistent with Scattered Stellar Light

Kavli Affiliate: Gregory J. Herczeg | First 5 Authors: Yifan Zhou, Brendan P. Bowler, Haifeng Yang, Aniket Sanghi, Gregory J. Herczeg | Summary: The proposed protoplanet AB Aur b is a spatially concentrated emission source imaged in the mm-wavelength disk gap of the Herbig Ae/Be star AB Aur. Its near-infrared spectrum and absence of strong […]


Continue.. UV-Optical Emission of AB Aur b is Consistent with Scattered Stellar Light

On the dominant role of wind in the quasar feedback mode in the late stage evolution of massive elliptical galaxies

Kavli Affiliate: Yingjie Peng | First 5 Authors: , , , , | Summary: In this paper we investigate the role of AGN feedback on the late stage evolution of elliptical galaxies by performing high-resolution hydrodynamical simulation in the {it MACER} framework. By comparing models that take into account different feedback mechanisms, namely AGN and […]


Continue.. On the dominant role of wind in the quasar feedback mode in the late stage evolution of massive elliptical galaxies

A search for pulsars around Sgr A* in the first Event Horizon Telescope dataset

Kavli Affiliate: Lijing Shao | First 5 Authors: Pablo Torne, Kuo Liu, Ralph P. Eatough, Jompoj Wongphechauxsorn, James M. Cordes | Summary: The Event Horizon Telescope (EHT) observed in 2017 the supermassive black hole at the center of the Milky Way, Sagittarius A* (Sgr A*), at a frequency of 228.1 GHz ($lambda$=1.3 mm). The fundamental […]


Continue.. A search for pulsars around Sgr A* in the first Event Horizon Telescope dataset