On the cosmological constant, the KK mass scale, and the cut-off dependence in the dark dimension scenario

被引：9

作者：

Anchordoqui, Luis A. ^{[1
,2
,3
]}

Antoniadis, Ignatios ^{[4
,5
]}

Luest, Dieter ^{[6
,7
]}

Luest, Severin ^{[8
]}

机构：

[1] CUNY, Lehman Coll, Dept Phys & Astron, New York, NY 10468 USA

[2] CUNY, Grad Ctr, Dept Phys, New York, NY 10016 USA

[3] Amer Museum Nat Hist, Dept Astrophys, New York, NY 10024 USA

[4] Sorbonne Univ, CNRS, Lab Phys Theor & Hautes Energies LPTHE, 4 Pl Jussieu, F-75005 Paris, France

[5] Univ Liverpool, Dept Math Sci, Liverpool L69 7ZL, England

[6] Ludwig Maximilians Univ Munchen, Arnold Sommerfeld Ctr Theoret Phys, D-80333 Munich, Germany

[7] Werner Heisenberg Inst, Max Planck Inst Phys, Fohringer Ring 6, D-80805 Munich, Germany

[8] Univ Montpellier, CNRS, Lab Charles Coulomb L2C, F-34095 Montpellier, France

来源：

EUROPEAN PHYSICAL JOURNAL C | 2023年 / 83卷 / 11期

基金：

美国国家科学基金会;

关键词：

All Open Access; Gold; Green;

D O I：

10.1140/epjc/s10052-023-12206-2

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

In this short note we comment on the relation between the cosmological and the Kaluza-Klein mass scale in the dark dimension scenario [1], also in view of some recent claims [2] that would raise some doubts about the validity of this scenario. Here we argue that these claims have serious flaws and cannot be trusted.

引用

页数：3

共 19 条

[11]

Gonzalo E, 2022, Arxiv, DOI arXiv:2209.09249

[12] FORBIDDEN MASS RANGE FOR SPIN-2 FIELD-THEORY IN DESITTER SPACETIME [J].