Limits on stochastic magnetic fields: A defense of our paper | Zendy

Chiara Caprini | Zendy; Ruth Durrer | Zendy

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Limits on stochastic magnetic fields: A defense of our paper

Author(s) -

Chiara Caprini,

Ruth Durrer

Publication year - 2005

Publication title -

physical review. d. particles, fields, gravitation, and cosmology/physical review. d, particles, fields, gravitation, and cosmology

Language(s) - English

Resource type - Journals

eISSN - 1550-7998

pISSN - 1550-2368

DOI - 10.1103/physrevd.72.088301

Subject(s) - amplitude , physics , magnetic field , limit (mathematics) , production (economics) , work (physics) , field (mathematics) , gravitational wave , quantum electrodynamics , theoretical physics , classical mechanics , statistical physics , quantum mechanics , economics , mathematics , mathematical analysis , pure mathematics , macroeconomics

In their recent paper ``Faraday rotation of the cosmic microwave backgroundpolarization by a stochastic magnetic field'', Kosowsky et al. Phys.Rev. D71,043006 (2005) have commented about our paper [C.Caprini and R.Durrer, Phys.Rev. D65, 023517 (2002)], in which we derived very strong limits on theamplitude of a primordial magnetic field from gravitational wave production.They argue that our limits are erroneous. In this short comment we defend ourresult.Comment: 2 pages, no figure

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