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researcher

M. Chu

4 papers hereh-index 7201 citations9 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.CO1
same name
  • M. Chu — 74 papers, h 49
  • M. Chu — 47 papers, h 26
  • M. Chu — 22 papers, h 7
  • M. Chu — 18 papers, h 2
  • M. Chu — 17 papers, h 26
  • M. Chu — 15 papers, h 35

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20022012
most citedGravitational Waves from Phase-Transition Induced Collapse of Neutron Stars

58 citations · 83 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.CO2012★ 14 cited

Cosmic histories of star formation and reionization: An analysis with a power-law approximation

Yun-Wei Yu, K. S. Cheng, M. C. Chu +1

With a simple power-law approximation of high-redshift (≳3.5) star formation history, i.e., ρ˙​∗​(z)∝[(1+z)/4.5]−α, we investigate the reionization of interga…

astro-ph2005★ 58 cited

Gravitational Waves from Phase-Transition Induced Collapse of Neutron Stars

L. -M. Lin, K. S. Cheng, M. -C. Chu +1

(Abridged) We study the gravitational radiation from gravitational collapses of rapidly rotating neutron stars induced by a phase-transition from normal nuclear matter to a mixed p…

astro-ph2003★ 1 cited

Gravitational Waves from Phase-Transition Induced Collapses of Neutron Stars

Lap-Ming Lin, Kwong-Sang Cheng, Wai-Mo Suen +1

We study the gravitational wave signals emitted from phase-transition induced collapses of rapidly rotating neutron stars to strange stars by performing 3D numerical simulations. O…

astro-ph2002★ 10 cited

Cooling Properties of Cloudy Bag Strange Stars

C. Y. Ng, K. S. Cheng, M. C. Chu

As the chiral symmetry is widely recognized as an important driver of the strong interaction dynamics, current strange stars models based on MIT bag models do not obey such symmetr…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.