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14 May 2018: called a Nakanishi–Lautrup field) and write. [f ] =. ZDh eSgf [h,r]/ , (8.24). ... representation, h 2 0M (g). This does not imply that (8.24) is gauge invariant: indeed itcannot be if it is to fix a gauge!

27 Feb 2018: Resource-explicit models of bacterial mutualismscompare well with experiments in which mutualists are wellmixed [5,6,23,24].

8 Aug 2018: capillary waves in thepresence of coexisting monolayer phases.24 The more gen-eral treatment of boundary motion applicable to a domain ofany shape has, however, remained an open problem of ... un5 24. ph8. n2. 4n221fn unu>2!, 35! when the subfluid

16 Jul 2018: Phys. Fluids 24, 061901 (2012). 18. Lauga, E. Bacterial hydrodynamics. Annu. ... 24. Johnson, R. E. An improved slender-body theory for Stokes flow.

23 May 2018: Iserles (ed.), Acta Numerica 24, Cambridge Univ. Press (2015). A. Iserles (ed.), Acta Numerica 23, Cambridge Univ.

11 Jan 2018: coli) [24], and also Salmonella typhimurium [23], Halobacteriumsalinarium [25], and Bacillus subtilis [26] [see Fig. ... 24). The terms on the left-hand side can be simplified by noting that.

19 Jul 2018: Thus the space oforbits of K2 in MC admits a Toda Einstein–Weyl structure [3, 24].• There exists a combination of self-dual two-forms which is degenerate when the harmonic. ... Roy. Soc. A363 (1978) 289–295.24. R. S. Ward, ‘Einstein-Weyl spaces

13 Dec 2018: As an illustration of the method, Figure 1 shows comparisons between the firstand second iterations of the operator series with ’exact’ computations from (24 ),restricted to the rough portion of the ... αr r′. = f(r,r′) (24). the expression (23)

3 Apr 2018: with (2.17).Finally, equation (2.24) is satisfied upon eliminating fww in the sameway and using w. ( ... 24. motion of N-vortices. There are several ways to obtain the metric forboth flat and curved backgrounds [46, 16].

23 Jan 2018: qq′). (1.24). Upon the substitution p′ = p m(qq′). t this becomes. ... Z0[J] =. d[ϕ] e. i2. ddx (µϕ(x)µϕ(x)m. 2ϕ2(x))iddx J(x)ϕ(x). (2.24). This is an integral with a highly oscillating integrand; if