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• W2018576556 abstract "We construct cosmological spacetimes with null Kasner-like singularities as purely gravitational solutions with no other background fields turned on. These can be recast as anisotropic plane-wave spacetimes by coordinate transformations. We analyze string quantization to find the spectrum of string modes in these backgrounds. The classical string modes can be solved for exactly in these time-dependent backgrounds, which enables a detailed study of the near-singularity string spectrum, (time-dependent) oscillator masses, and wave functions. We find that for low-lying string modes (finite oscillation number), the classical near-singularity string mode functions are nondivergent for various families of singularities. Furthermore, for any infinitesimal regularization of the vicinity of the singularity, we find a tower of string modes of ultrahigh oscillation number which propagate essentially freely in the background. The resulting picture suggests that string interactions are non-negligible near the singularity." @default.
• W2018576556 created "2016-06-24" @default.
• W2018576556 creator A5066664176 @default.
• W2018576556 creator A5075359028 @default.
• W2018576556 date "2009-06-15" @default.
• W2018576556 modified "2023-09-25" @default.
• W2018576556 title "String spectra near some null cosmological singularities" @default.
• W2018576556 cites W1596494754 @default.
• W2018576556 cites W1843094897 @default.
• W2018576556 cites W1963684035 @default.
• W2018576556 cites W1966856415 @default.
• W2018576556 cites W1970265338 @default.
• W2018576556 cites W1977718304 @default.
• W2018576556 cites W1982661754 @default.
• W2018576556 cites W1984160218 @default.
• W2018576556 cites W1988304627 @default.
• W2018576556 cites W1990973510 @default.
• W2018576556 cites W1998364811 @default.
• W2018576556 cites W2003317037 @default.
• W2018576556 cites W2003909464 @default.
• W2018576556 cites W2006029361 @default.
• W2018576556 cites W2007211812 @default.
• W2018576556 cites W2008907874 @default.
• W2018576556 cites W2009023037 @default.
• W2018576556 cites W2009068975 @default.
• W2018576556 cites W2010228656 @default.
• W2018576556 cites W2010747229 @default.
• W2018576556 cites W2012687263 @default.
• W2018576556 cites W2022174740 @default.
• W2018576556 cites W2022955804 @default.
• W2018576556 cites W2030375488 @default.
• W2018576556 cites W2039177077 @default.
• W2018576556 cites W2039553496 @default.
• W2018576556 cites W2043260986 @default.
• W2018576556 cites W2045010570 @default.
• W2018576556 cites W2048737175 @default.
• W2018576556 cites W2048815852 @default.
• W2018576556 cites W2050086929 @default.
• W2018576556 cites W2050552037 @default.
• W2018576556 cites W2051527080 @default.
• W2018576556 cites W2051815668 @default.
• W2018576556 cites W2052064015 @default.
• W2018576556 cites W2053772722 @default.
• W2018576556 cites W2054108292 @default.
• W2018576556 cites W2056845750 @default.
• W2018576556 cites W2057938013 @default.
• W2018576556 cites W2066166718 @default.
• W2018576556 cites W2066472473 @default.
• W2018576556 cites W2068225248 @default.
• W2018576556 cites W2068995422 @default.
• W2018576556 cites W2071491215 @default.
• W2018576556 cites W2073268899 @default.
• W2018576556 cites W2080831749 @default.
• W2018576556 cites W2083999055 @default.
• W2018576556 cites W2089209281 @default.
• W2018576556 cites W2089669092 @default.
• W2018576556 cites W2090615656 @default.
• W2018576556 cites W2105981695 @default.
• W2018576556 cites W2113445082 @default.
• W2018576556 cites W2118842899 @default.
• W2018576556 cites W2143598364 @default.
• W2018576556 cites W2145944908 @default.
• W2018576556 cites W2149671832 @default.
• W2018576556 cites W2159703566 @default.
• W2018576556 cites W2165154082 @default.
• W2018576556 cites W2168477707 @default.
• W2018576556 cites W2950493112 @default.
• W2018576556 cites W2997401925 @default.
• W2018576556 cites W3037256083 @default.
• W2018576556 cites W3098142195 @default.
• W2018576556 cites W3098568217 @default.
• W2018576556 cites W3098784140 @default.
• W2018576556 cites W3099027764 @default.
• W2018576556 cites W3099152290 @default.
• W2018576556 cites W3099520568 @default.
• W2018576556 cites W3099697639 @default.
• W2018576556 cites W3099975630 @default.
• W2018576556 cites W3100235408 @default.
• W2018576556 cites W3102010038 @default.
• W2018576556 cites W3102060593 @default.
• W2018576556 cites W3102065702 @default.
• W2018576556 cites W3102109419 @default.
• W2018576556 cites W3102316661 @default.
• W2018576556 cites W3102479198 @default.
• W2018576556 cites W3102699341 @default.
• W2018576556 cites W3103180817 @default.
• W2018576556 cites W3103489229 @default.
• W2018576556 cites W3103953580 @default.
• W2018576556 cites W3104026949 @default.
• W2018576556 cites W3104143950 @default.
• W2018576556 cites W3104573932 @default.
• W2018576556 cites W3104742972 @default.
• W2018576556 cites W3105191441 @default.
• W2018576556 cites W3105560651 @default.
• W2018576556 cites W3105812440 @default.
• W2018576556 cites W47131799 @default.
• W2018576556 doi "https://doi.org/10.1103/physrevd.79.126009" @default.
• W2018576556 hasPublicationYear "2009" @default.
• W2018576556 type Work @default.
• W2018576556 sameAs 2018576556 @default.

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