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Jaffe AH Ade PA Balbi A Bock JJ Bond JR Borrill J Boscaleri A Coble K Crill BP de Bernardis P Farese P Ferreira PG Ganga K Giacometti M Hanany S Hivon E Hristov VV Iacoangeli A Lange AE Lee AT Martinis L Masi S Mauskopf PD Melchiorri A Montroy T Netterfield CB Oh S Pascale E Piacentini F Pogosyan D Prunet S Rabii B Rao S Richards PL Romeo G Ruhl JE Scaramuzzi F Sforna D Smoot GF Stompor R Winant CD Wu JH 《Physical review letters》2001,86(16):3475-3479
Recent results from BOOMERANG-98 and MAXIMA-1, taken together with COBE DMR, provide consistent and high signal-to-noise measurements of the cosmic microwave background power spectrum at spherical harmonic multipole bands over 2相似文献
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To accommodate the observed accelerated expansion of the universe, one popular idea is to invoke a driving term in the Friedmann–Lemaître equation of dark energy which must then comprise 70% of the present cosmological energy density. We propose an alternative interpretation which takes into account the entropy and temperature intrinsic to the horizon of the universe due to the information holographically stored there. Dark energy is thereby obviated and the acceleration is due to an entropic force naturally arising from the information storage on the horizon surface screen. We consider an additional quantitative approach inspired by surface terms in general relativity and show that this leads to the entropic accelerating universe. 相似文献