{
  "annotation_id": "6887d661-0bef-4c0a-b67c-77073900bae7",
  "date_created": "2026-02-17T05:53:23.748000Z",
  "date_modified": "2026-02-17T05:53:23.748000Z",
  "file_hash": "e090550ceb341267609339b919f8c4292afc15c1e80f0508c3609f7a8254af7d",
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  "record": {
    "abstract": "We summarize the current state of the art and calculate gravitational wave strain amplitudes for known binary pulsars, using data from current ground-based detectors (LIGO-Virgo-KAGRA) and the upcoming space-based missions (LISA). We present detailed calculations of the characteristic gravitational wave strain values, ranging from 3.0 to 73 $\\times10^{-22}$, across frequencies between 0.66 and 5.87 $\\times10^{-4}$ Hz. Our post-Newtonian approximation analysis yields predicted periastron advance rates from 1.6 to 80.5 deg/yr and orbital period decay rates between -5 and -176 $\\mu$s/yr for the binary pulsar population. We derive common envelope efficiency parameters ($\\alpha_{CE}$) for representative progenitor scenarios within our sample, finding values between 0.63 and 1.16, with notable sensitivity to the binding energy parameter $\\lambda$. Binary neutron star merger rates are estimated at $22.77^{+6.83}_{-6.83}$ Myr$^{-1}$ for the Milky Way, corresponding to a volumetric rate of $227.71^{+68.31}_{-68.31}$ Gpc$^{-3}$ yr$^{-1}$, consistent with the latest LIGO-Virgo-KAGRA observational constraints. Our results illustrate how multi-band gravitational wave observations, from LIGO/Virgo to LISA, can contribute to precise measurements of binary pulsar strain and orbital evolution histories, improving merger time predictions and constraining neutron star physics and common envelope processes",
    "arxiv_id": "2601.09863",
    "authors": [
      "Ali Taani"
    ],
    "categories": [
      "astro-ph.HE"
    ],
    "doi": "10.1140/epjp/s13360-025-07084-4",
    "journal_ref": "The European Physical Journal Plus 141, 2026, (1), 21",
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "title": "Gravitational Wave Strain and Orbital Dynamics of Binary Pulsars from LIGO-Virgo to LISA",
    "url": "https://arxiv.org/abs/2601.09863",
    "version": "v1"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "efb867f0-f0d5-4583-b721-0b566dea2cad",
    "id": "arXiv Dataset",
    "type": "Model",
    "variant": "snapshot-2026-01-17",
    "version": "0.1.0"
  },
  "user_id": 1000002
}