These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
147 related articles for article (PubMed ID: 10991377)
1. Limit on primordial small-scale magnetic fields from cosmic microwave background distortions. Jedamzik K; Katalinic V; Olinto AV Phys Rev Lett; 2000 Jul; 85(4):700-3. PubMed ID: 10991377 [TBL] [Abstract][Full Text] [Related]
2. Cosmic microwave background trispectrum and primordial magnetic field limits. Trivedi P; Seshadri TR; Subramanian K Phys Rev Lett; 2012 Jun; 108(23):231301. PubMed ID: 23003943 [TBL] [Abstract][Full Text] [Related]
3. Cosmic microwave background bispectrum from primordial magnetic fields on large angular scales. Seshadri TR; Subramanian K Phys Rev Lett; 2009 Aug; 103(8):081303. PubMed ID: 19792712 [TBL] [Abstract][Full Text] [Related]
4. Reheating the universe once more: the dissipation of acoustic waves as a novel probe of primordial inhomogeneities on even smaller scales. Nakama T; Suyama T; Yokoyama J Phys Rev Lett; 2014 Aug; 113(6):061302. PubMed ID: 25148314 [TBL] [Abstract][Full Text] [Related]
5. Stringent Limit on Primordial Magnetic Fields from the Cosmic Microwave Background Radiation. Jedamzik K; Saveliev A Phys Rev Lett; 2019 Jul; 123(2):021301. PubMed ID: 31386540 [TBL] [Abstract][Full Text] [Related]
6. Taking the Universe's Temperature with Spectral Distortions of the Cosmic Microwave Background. Hill JC; Battaglia N; Chluba J; Ferraro S; Schaan E; Spergel DN Phys Rev Lett; 2015 Dec; 115(26):261301. PubMed ID: 26764983 [TBL] [Abstract][Full Text] [Related]
7. Can cosmic shear shed light on low cosmic microwave background multipoles? Kesden M; Kamionkowski M; Cooray A Phys Rev Lett; 2003 Nov; 91(22):221302. PubMed ID: 14683227 [TBL] [Abstract][Full Text] [Related]
8. Estimate of the primordial magnetic field helicity. Vachaspati T Phys Rev Lett; 2001 Dec; 87(25):251302. PubMed ID: 11736556 [TBL] [Abstract][Full Text] [Related]
9. Cosmic microwave background polarization signals from tangled magnetic fields. Seshadri TR; Subramanian K Phys Rev Lett; 2001 Sep; 87(10):101301. PubMed ID: 11531471 [TBL] [Abstract][Full Text] [Related]
10. Relieving the Hubble Tension with Primordial Magnetic Fields. Jedamzik K; Pogosian L Phys Rev Lett; 2020 Oct; 125(18):181302. PubMed ID: 33196251 [TBL] [Abstract][Full Text] [Related]
11. The origin, evolution and signatures of primordial magnetic fields. Subramanian K Rep Prog Phys; 2016 Jul; 79(7):076901. PubMed ID: 27243368 [TBL] [Abstract][Full Text] [Related]
12. Scientific results from the Cosmic Background Explorer (COBE). Bennett CL; Boggess NW; Cheng ES; Hauser MG; Kelsall T; Mather JC; Moseley SH; Murdock TL; Shafer RA; Silverberg RF; Smoot GF; Weiss R; Wright EL Proc Natl Acad Sci U S A; 1993 Jun; 90(11):4766-73. PubMed ID: 11607383 [TBL] [Abstract][Full Text] [Related]
13. Are cluster magnetic fields primordial? Banerjee R; Jedamzik K Phys Rev Lett; 2003 Dec; 91(25):251301. PubMed ID: 14754103 [TBL] [Abstract][Full Text] [Related]
14. Can primordial magnetic fields be the origin of the BICEP2 data? Bonvin C; Durrer R; Maartens R Phys Rev Lett; 2014 May; 112(19):191303. PubMed ID: 24877927 [TBL] [Abstract][Full Text] [Related]
15. Implications of a primordial origin for the dispersion in D/H in quasar absorption systems. Copi CJ; Olive KA; Schramm DN Proc Natl Acad Sci U S A; 1998 Mar; 95(6):2758-60. PubMed ID: 9501162 [TBL] [Abstract][Full Text] [Related]
16. Generation of primordial magnetic fields on linear overdensity scales. Naoz S; Narayan R Phys Rev Lett; 2013 Aug; 111(5):051303. PubMed ID: 23952384 [TBL] [Abstract][Full Text] [Related]
17. New window on primordial non-gaussianity. Pajer E; Zaldarriaga M Phys Rev Lett; 2012 Jul; 109(2):021302. PubMed ID: 23030152 [TBL] [Abstract][Full Text] [Related]