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Fifth Force

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lightbulbAbout this topic
The Fifth Force refers to a hypothetical fundamental force of nature beyond the four known forces (gravitational, electromagnetic, strong nuclear, and weak nuclear). It is proposed to explain phenomena not accounted for by existing theories, potentially involving new particles or interactions that could reshape our understanding of physics.
lightbulbAbout this topic
The Fifth Force refers to a hypothetical fundamental force of nature beyond the four known forces (gravitational, electromagnetic, strong nuclear, and weak nuclear). It is proposed to explain phenomena not accounted for by existing theories, potentially involving new particles or interactions that could reshape our understanding of physics.

Key research themes

1. How do experimental tests probe composition-dependent fifth forces and what are the implications of historic data reanalyses?

This theme focuses on the experimental search for fifth forces that depend on the composition of test masses, primarily using precision tests of the Weak Equivalence Principle (WEP). It evaluates historical experiments and modern reinterpretations to assess evidence of composition-dependent forces, the methodological requirements for robust detection, and implications for new physics beyond gravity.

Key finding: The reanalysis of the 1904-1908 Eötvös, Pekár, and Fekete (EPF) data reveals a significant correlation between acceleration differences and baryon-to-mass ratios of test samples, suggesting a possible composition-dependent... Read more
Key finding: Through reanalysis of Potter's 1923 pendulum experiment data, the study uncovers a pattern in period differences correlated with baryon-to-mass ratios, implying a fifth force coupling to baryon number. This challenges the... Read more
Key finding: This review distills a decade of searches for a gravity-like fifth force characterized by a Yukawa potential with strength α and range λ. It systematizes constraints from composition-dependent and composition-independent... Read more

2. How can modern interferometric and precision magnetometry methods constrain spin-dependent and axion-mediated fifth forces?

This research area explores experimental strategies that exploit neutron interferometry and precision magnetometry to detect or constrain exotic fifth forces mediated by ultralight axion-like particles and spin-dependent interactions. By focusing on specific particle-mediated forces and exploiting spin-mass couplings, these methods offer complementary approaches to traditional gravitational tests, targeting new parameter space regions with high sensitivity.

Key finding: This paper proposes a novel neutron interferometric method to detect fermion–fermion interactions mediated by axions or axion-like particles (ALPs). By splitting a neutron beam into two paths exposed to differently oriented... Read more
Key finding: Using room temperature lead masses and a paramagnetic crystal cooled to 4.2 K probed by a SQUID-based magnetometer with 53 aT/Hz sensitivity, the experiment sets unprecedented constraints on spin-mass axion-mediated forces... Read more

3. What roles do modified gravity theories with screening mechanisms and fifth force phenomenology play in astrophysical and cosmological tests?

This theme encompasses investigations of theoretical models extending General Relativity with additional scalar fields or nonminimal curvature-matter couplings that induce fifth forces, possibly screened in high-density environments. It includes the development of phenomenological frameworks and surrogate models facilitating rapid predictions for astrophysical systems (binary pulsars, gravitational wave sources) and cosmological large-scale structure, providing pathways to constrain or detect new gravitational physics with current and upcoming observations.

Key finding: The study formulates the tree-level three-point correlation function (3PCF) of biased tracers under Modified Gravity (MG) theories with scale-dependent gravitational strength, focusing on Hu-Sawicky f(R) and DGP models... Read more
Key finding: This work derives analytic expressions for orbital period decay in compact binaries subject to a fifth force mediated by ultralight bosons and additional radiation of these particles, incorporating effects of orbital... Read more
Key finding: By extending analysis of nonminimally coupled curvature-matter gravity models featuring both Yukawa-type fifth forces and additional non-Newtonian forces related to spatial gradients of curvature, the study shows that Solar... Read more
Key finding: The research identifies massive Galileon scalar-tensor theories exhibiting Vainshtein screening at the classical effective level, demonstrating suppression of an extra scalar-mediated fifth force near compact sources.... Read more
Key finding: The authors develop a reduced order surrogate model (pySTGROMX) for the Damour-Esposito-Farèse (DEF) scalar-tensor gravity theory, incorporating spontaneous scalarization effects in neutron stars. The surrogate enables rapid... Read more

All papers in Fifth Force

We introduce a new framework for cosmic acceleration: the Scalar-Cost Dark Energy model. In this approach, dark energy arises not from a cosmological constant but from an energetic cost associated with the expansion of spacetime. This... more
The suggestion in 1986 of a possible gravity-like ``fifth" fundamental force renewed interest in the question of whether new macroscopic forces are present in nature. Such forces are predicted in many theories which unify gravity with the... more
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We develop a falsifiable framework in which the phenomenon attributed to "dark matter" arises from resonant overlap shadows cast by the baryonic sector, of which only ~15% is directly visible (luminous stars, gas, dust). Here a shadow... more
The electromagnetic force, strong nuclear force, weak nuclear force, and gravitational force are the four fundamental forces of nature. The Standard Model (SM) succeeded in combining the first three forces to describe the most basic... more
All the four fundamental forces of nature have been explained in terms of space time. Coupling constant of grand unification has been defined by space time. The density of space time calculated by 'Siva's classical equation for space... more
All the four fundamental forces of nature have been explained in terms of space time. Coupling constant of grand unification has been defined by space time. The density of space time calculated by 'Siva's classical equation for space... more
We propose a new table-top experimental configuration for the direct detection of dark matter QCD axions in the traditional open mass window 10 -6 eV ma 10 -2 eV using non-perturbative effects in a system with non-trivial spatial... more
In this paper, we analyze the importance of the fields: Yukawa (nuclear level), Bohr (atomic level), Planck (Universe level-non human) and Schwinger (void structure). The interrelations of these fields guarantee the stability of the... more
In real Einstein-Lifts above resp. in radial gravitational-fields over planetary surfaces there appear tidal forces, which causes small deviations from real inertial systems because the Ricci-Tensor in the Lift is not equal to zero,... more
Weakly interactive slim particles (WISPs), including the QCD axion, axion-like particles (ALPs), and hidden photons, are considered to be strong candidates for the dark matter carrier particle. The microwave cavity experiment WISPDMX is... more
Se propone una hipótesis teórica que vincula estructuras de flujo hidrodinámico en vórtices de Rankine confinados con materiales de topología exótica como el hexaboruro de samario (SmB), planteando la posibilidad de interpretar el eje de... more
Dark photons are particles invoked in some extensions of the Standard Model that could account for at least part of the dark matter content of the Universe. It has been proposed that the production of dark photons in stellar interiors... more
Theories that attempt to explain the observed cosmic acceleration by modifying general relativity all introduce a new scalar degree of freedom that is active on large scales, but is screened on small scales to match experiments. We... more
Abstract: An alternative quantization method of local fields was proposed in the papers [1, 2] (cf.: [3]). In this paper we discuss three cosmological aspects in connection with this quantization method called quantum local field theory... more
Indications of a possible composition-dependent fifth force, based on a reanalysis of the Eötvös experiment, have not been supported by a number of modern experiments. Here, we argue that searching for a composition-dependent fifth force... more
We have reanalyzed data obtained by Potter in a 1923 experiment aimed at testing whether the accelerations of test masses in the Earth's gravitational field are independent of their compositions. Although Potter concludes that the... more
Employing unique and proprietary circuitry to produce a closed-loop amplifier system which features exceptional DC stability and excellent wideband performance characteristics.
DOI: will be assigned Measurements in the radio regime embrace a number of effective approaches for WISP searches, often covering unique or highly complementary ranges of the parameter space compared to those explored in other research... more
The physics case for axions and axion-like particles is reviewed and an overview of ongoing and near-future laboratory searches is presented.
Many theoretically well-motivated extensions of the Standard Model of particle physics predict the existence of the axion and further ultralight axion-like particles. They may constitute the mysterious dark matter in the universe and... more
The division of galaxies into "barred" (SB) and "normal" (S) spirals is a fundamental aspect of the Hubble galaxy classification system. This "tuning fork" view was revised by de Vaucouleurs, whose classification volume recognized... more
A new search strategy for the detection of the elusive dark matter (DM) axion is proposed. The idea is based on streaming DM axions, whose flux might get temporally enormously enhanced due to gravitational lensing. This can happen if the... more
Light scalar fields can drive accelerated expansion of the universe. Hence, scalars are obvious dark energy candidates. To make these models compatible with test of General Relativity in the solar system and fifth force searches on earth,... more
We consider a nonminimally coupled curvature-matter gravity theory at the Solar System scale. Both a fifth force of Yukawa type and a further non-Newtonian extra force that arises from the nonminimal coupling are present in the solar... more
We study a theory of gravity in which the action is a result from the general purely disformal transformation on the Einstein-Hilbert action. This theory is a sub-class of GLPV theory which is the the generalization of covariant Galileon.... more
We review the experimental constraints on additional macroscopic Yukawa forces for interaction ranges below 1 cm, and summarize several theoretical predictions of new forces in this region. An experiment using 1 kHz mechanical oscillators... more
We study spherical collapse in the Quartic and Quintic Covariant Galileon gravity models within the framework of the excursion set formalism. We derive the nonlinear spherically symmetric equations in the quasi-static and weak-field... more
This review is a pedagogical introduction to models of gravity and how they are constrained through cosmological observations. We focus on the Horndeski scalar-tensor theory and on the quantities that can be measured with a minimum of... more
We discuss the problem of constructing models containing an axion and axion-like particles, motivated by astrophysical observations, with decay constants at the intermediate scale ranging from $10^9$GeV to $10^{13}$GeV. We present... more
We consider possibilities to grasp and drag one-dimensional solitons in two-component Bose–Einstein condensates (BECs), under the action of gravity, by tweezers induced by spatially confined spin–orbit (SO) coupling applied to the BEC,... more
The relation between the activity of cells in the motor cortex and static force has been studied extensively. Most studies have concentrated on the relation to the magnitude of force; this relation is more or less monotonic. The slope of... more
When the Abraham Lorentz force is considered in the context of two independently interacting charged particles a surprising consequence arises where particles will feel an Abraham Lorentz force that is creates an attractive force between... more
The next generation of galaxy surveys will provide highly accurate measurements of the largescale structure of the Universe, allowing for more stringent tests of gravity on cosmological scales. Higher order statistics are a valuable tool... more
A scale invariant model containing dilaton φ and dust (as a model of matter) is studied where the shift symmetry φ → φ + const. is spontaneously broken at the classical level due to intrinsic features of the model. The dilaton to matter... more
Dark sectors, consisting of new, light, weakly-coupled particles that do not interact with the known strong, weak, or electromagnetic forces, are a particularly compelling possibility for new physics. Nature may contain numerous dark... more
Dark matter Axion search with riNg Cavity Experiment (DANCE) was proposed. To search for axion-like particles, we aim to detect the rotation and oscillation of optical linear polarization caused by axion-photon coupling with a bow-tie... more
We obtain constraints on non-Newtonian gravity following from the improved precision measurement of the Casimir force by means of atomic force microscope. The hypothetical force is calculated in experimental configuration (a sphere above... more
On large cosmological scales, anisotropic gravitational collapse is manifest in the dark cosmic web. Its statistical properties are little known for alternative dark matter (DM) models such as fuzzy dark matter (FDM). In this work, we... more
On large cosmological scales, anisotropic gravitational collapse is manifest in the dark cosmic web. Its statistical properties are little known for alternative dark matter models such as fuzzy dark matter (FDM). In this work, we assess... more
The International Axion Observatory (IAXO) is a forth generation axion helioscope designed to detect solar axions and axion-like particles (ALPs) with a coupling to the photon g aγ down to a few 10 −12 GeV −1 , 1.5 orders of magnitude... more
We present an analysis of the anomalous grawtatlonal attracuon found in the Greenland lcesheet experiment If the anomalous gra&ent ~s due to the existence of a single new, attractive, force, then the force has a range between 225 m and 5... more
It is shown that dark matter axions cause an oscillating electric current to flow along magnetic field lines. The oscillating current induced in a strong magnetic field B0 produces a small magnetic field Ba. We propose to amplify and... more
The LHAASO Collaboration has reported their observation of very high energy photons (E max γ ≃ 18 TeV) from the gamma-ray burst GRB221009A. The sterile neutrino that involves both mixing and a transition magnetic moment may be a viable... more
Newtonian simulations are routinely used to examine the matter dynamics on non-linear scales. However, even on these scales, Newtonian gravity is not a complete description of gravitational effects. A post-Friedmann approach shows that... more
We consider effective model where photons interact with scalar field corresponding to conformal excitations of the internal space (geometrical moduli/gravexcitons). We demonstrate that this interaction results in a modified dispersion... more
During galactic Supernova (SN) explosions, a large amount of feebly interacting particles (FIPs) may be produced. In this work we analyze electrophilic FIPs with masses in the MeV-range that escape from SN and decay into electron-positron... more
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