• Title of article

    Lunar seismic search for strange quark matter Original Research Article

  • Author/Authors

    M. Casolino، نويسنده , , M.P. De Pascale، نويسنده , , M. Nagni، نويسنده , , P. Picozza، نويسنده ,

  • Issue Information
    دوهفته نامه با شماره پیاپی سال 2006
  • Pages
    5
  • From page
    1889
  • To page
    1893
  • Abstract
    It was pointed out in 1984 by Witten that strange quark matter (SQM) – matter made of up, down, and strange quarks (rather than just up and down, as are protons and neutrons) – might well be stable and the lowest energy state of matter. The reason is that it would be electrically neutral and have less Pauli-Principle repulsion. Binding would increase with numbers of quarks, and might not begin below thousands. It would have nuclear density. Neutron stars would be strange quark stars; and it might conceivably constitute dark matter. One way to detect ton-range SQM nuggets (SQNs) would be from seismic signals they would make passing through the Earth. We give a rough estimate on the relative advantage of attempting to detect SQNs on the Moon over Earth (about 50 times more detections).
  • Keywords
    Moon , Strange quark matter , Seismic detection
  • Journal title
    Advances in Space Research
  • Serial Year
    2006
  • Journal title
    Advances in Space Research
  • Record number

    1130885