activity
20102026
most citedGravitational wave searches for ultralight bosons with LIGO and LISA

345 citations · 1.5k across the 33 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2024★ 18 cited

Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels

Boyuan Liu, Tilman Hartwig, Nina S. Sartorio +6

The gravitational wave (GW) signal from binary black hole (BBH) mergers is a promising probe of Population III (Pop III) stars. To fully unleash the power of the GW probe, one impo…

astro-ph.GA2020★ 106 cited

Massive black hole merger rates: the effect of kpc separation wandering and supernova feedback

Enrico Barausse, Irina Dvorkin, Michael Tremmel +2

We revisit the predictions for the merger rate of massive black hole binaries detectable by the Laser Interferometer Space Antenna (LISA) and their background signal for pulsar-tim…

astro-ph.GA2017★ 24 cited

Cosmological evolution of the Nitrogen abundance

Elisabeth Vangioni, Irina Dvorkin, Keith A. Olive +5

The abundance of nitrogen in the interstellar medium is a powerful probe of star for- mation processes over cosmological timescales. Since nitrogen can be produced both in massive…

astro-ph.GA2017★ 43 cited

The nightmare scenario: measuring the stochastic gravitational-wave background from stalling massive black-hole binaries with pulsar-timing arrays

Irina Dvorkin, Enrico Barausse

Massive black-hole binaries, formed when galaxies merge, are among the primary sources of gravitational waves targeted by ongoing Pulsar Timing Array (PTA) experiments and the upco…

astro-ph.GA2016★ 23 cited

Evolution of dispersion in the cosmic deuterium abundance

Irina Dvorkin, Elisabeth Vangioni, Joseph Silk +2

Deuterium is created during Big Bang Nucleosynthesis, and, in contrast to the other light stable nuclei, can only be destroyed thereafter by fusion in stellar interiors. In this pa…

astro-ph.GA2014★ 13 cited

Evolution of the gas mass fraction in galaxy clusters

Irina Dvorkin, Yoel Rephaeli

The mass fraction of hot gas in clusters is a basic quantity whose level and dependence on the cluster mass and redshift are intimately linked to all cluster X-ray and SZ measures.…