DOI: 10.1140/epjc/s10052-026-15933-4 ISSN: 1434-6052

Hyperbolic form factors for Yukawa interactions, and applications to the Earth

Pierre Fayet

Abstract

We define the hyperbolic form factor of a density distribution as its bilateral Laplace transform, related by duality or analytic continuation to its ordinary form factor.  For a sphere it is given by

$$\Phi (x \!= \! kR) =\langle \,\cosh \,\vec k.\vec r\,\rangle = \langle \,\frac{\sinh kr}{kr}\,\rangle $$ Φ ( x = k R ) = ⟨ cosh k → . r → ⟩ = ⟨ sinh k r kr ⟩
, expanded as
$$\,\sum _0^\infty \frac{x^{2n}}{(2n+1)! }\, \frac{\langle r^{2n}\rangle }{R^{2n}}$$ ∑ 0 ∞ x 2 n ( 2 n + 1 ) ! ⟨ r 2 n ⟩ R 2 n
, and similarly for the form factor
$$ \langle \,\frac{\sin kr}{kr}\,\rangle $$ ⟨ sin k r kr ⟩
. It is also obtained from the bilateral Laplace transform of
$$2\pi r\,\rho (|r|)$$ 2 π r ρ ( | r | )
, and enters in the determination of the outside Yukawa potential induced by a new charge for a mediator of mass
$$m= k=$$ m = k =
$$1/\lambda $$ 1 / λ
.  
$$\Phi (x)$$ Φ ( x )
may be expressed as
$$\frac{3}{x^3}\,(x\,\cosh x - \sinh x) \times {{\bar{\rho }}} (x)/\rho _0$$ 3 x 3 ( x cosh x - sinh x ) × ρ ¯ ( x ) / ρ 0
, where
$${{\bar{\rho }}}(x)$$ ρ ¯ ( x )
is an effective density decreasing (for
$$d\rho /dr <0)$$ d ρ / d r < 0 )
from the average
$$\rho _0$$ ρ 0
at small x , down to the density
$$\rho (R)$$ ρ ( R )
near the surface. An inversion formula allows one to recover the density distribution
$$\rho (r)$$ ρ ( r )
from an analytic continuation of
$$\Phi (x)$$ Φ ( x )
, as
$$\rho (r) =\rho _0\, (2R/3\pi r)\int _0^\infty \Phi (ix) \, \sin (x\frac{r}{R})\ x\,dx\,$$ ρ ( r ) = ρ 0 ( 2 R / 3 π r ) ∫ 0 ∞ Φ ( i x ) sin ( x r R ) x d x
.