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Why the cosmological constant problem is hard

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Publication:1579412
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DOI10.1016/S0370-2693(00)00901-1zbMath1050.83514arXivhep-th/0006059OpenAlexW3101430134WikidataQ125967184 ScholiaQ125967184MaRDI QIDQ1579412

N. Delaunay

Publication date: 6 September 2000

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0006059


zbMATH Keywords

bulk cosmological constantKaluza-Klein theorymass gapdistance scalelarge distancesbrane world scenariosbulk graviton mode spectrumcompletely broken supersymmetryDvali-Gabadadze-Porrati modeleffectively 4D theoryinfinite volume extra dimensionsnonzero brane cosmological constantsupersymmetric bulk


Mathematics Subject Classification ID

String and superstring theories in gravitational theory (83E30) Quantization of the gravitational field (83C45) Kaluza-Klein and other higher-dimensional theories (83E15)


Related Items (4)

A REMARK ON NONCONFORMAL NONSUPERSYMMETRIC THEORIES WITH VANISHING VACUUM ENERGY DENSITY ⋮ "SELF-TUNING" AND CONFORMALITY ⋮ SOLITONIC BRANE WORLD WITH COMPLETELY LOCALIZED (SUPER)GRAVITY ⋮ Gravity in Randall-Sundrum brane world revisited







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