A constraint on a varying proton–electron mass ratio 1.5 billion years after the Big Bang: Supplemental Material
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چکیده
0 7 W3R(0), L14R(0), L10R(0), L8R(0), L7R(0), L1R(0), L0R(0) 1 20 L16P(1), L15P(1), L15R(1), W3R(1), L12R(1), L12P(1), W2Q(1), L10R(1), L10P(1), L9R(1), L9P(1), L8P(1), L4R(1), L4P(1), L3R(1), L3P(1), L2R(1), L2P(1), L1R(1), L1P(1) 2 27 L16R(2), L15R(2), L13R(2), L12P(2), W2R(2), W2Q(2), W2P(2), L11R(2), L11P(2), L10P(2), W1R(2), W1Q(2), L9R(2), L9P(2), L8R(2), W0Q(2), L7R(2), L6P(2), L5P(2), L4R(2), L4P(2), L3P(2), L2R(2), L2P(2), L1R(2), L1P(2), L0P(2) 3 26 L15R(3), W3P(3), L13R(3), L13P(3), L12R(3), W2R(3), L12P(3), W2Q(3), W2P(3), L11P(3), L10R(3), L10P(3), W1R(3), L9R(3), W0R(3), W0Q(3), L6R(3), L5P(3), L4R(3), L4P(3), L3R(3), L3P(3), L2R(3), L1R(3), L0R(3) 4 9 L17P(4), L16P(4), L15R(4), L13P(4), L12R(4), L11P(4), W1Q(4), L9P(4), W0Q(4) CONTINUUM ERROR
منابع مشابه
Constraint on a varying proton-electron mass ratio 1.5 billion years after the big bang.
A molecular hydrogen absorber at a lookback time of 12.4 billion years, corresponding to 10% of the age of the Universe today, is analyzed to put a constraint on a varying proton-electron mass ratio, μ. A high resolution spectrum of the J1443+2724 quasar, which was observed with the Very Large Telescope, is used to create an accurate model of 89 Lyman and Werner band transitions whose relative ...
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