Outline
The theory of mechanics presented by Sir Isaac Newton in 1687 is the foundation of classical mechanics and modern physics. This article relates to his work by first considering velocity and acceleration. For EthnoPhysics, these dynamic concepts are logically defined from sensations, and quantified by measurement. Then we develop the notion of force based on Newton’s second law of motion. His first law is used to define straight lines and linear motion. And finally, Newton’s third law is interpreted as a scientific reiteration of venerable knowledge that can be traced back as far as the Vedic literature . These widespread ancient ideas about cause and effect are often referred to as karma .
Velocity
Consider a particle P described by a repetitive chain
of historically ordered space-time events
Let these events be characterized by their position
and time of occurrence
Then we write
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The separation between some arbitrary initial and final pair of events is given by
And the elapsed time between these events is
Then a velocity vector is defined by the ordered set of three numbers
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The speed of P is defined by the norm of the velocity
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Consider measuring this quantity based on observations of length and time. Recall that length is defined only for particles that are at least as big as atoms. And we also presume that P is compared to a frame of reference that includes a calibrated rod and a calibrated clock
To determine the velocity first measure the elapsed time between events
and
as
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where
is the number of clock cycles between initial and final events,
is the period and
is the frequency of P. Then make three length measurements along the spatial axes that are noted by
and
Combine these measurements to obtain the observed separation vector
between events which may be written as
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where
characterizes the motion of P during one complete orbital cycle
. As discussed earlier atomic cycles are separated from each other by one wavelength
And if measurements are not too disruptive so that
is constant, then the distance between initial and final events is
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Combining these observations gives the measured speed of P as
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If P contains many quarks we can use Planck’s postulate to substitute the mechanical energy
for the frequency to obtain
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And if the frame of reference is inertial then de Broglie’s postulate can be used to replace the wavelength with the momentum
to obtain
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The Speed of a Photon
If the particle under consideration is a graviton or a photon
then its mass
is zero, and its energy is given by
Substituting this into the expression for speed developed above gives
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And so the constant number
is usually called the speed of light. For photons
Thus the wavenumber
and other photon characteristics are all related as
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The Speed of a Newtonian Particle
If P is Newtonian then
and the particle is presumably in dynamic equilibrium with its environment. For this case, the mechanical energy is given by
where
is the kinetic energy. So for Newtonian particles
![]()
But recall that kinetic energy is defined by
So for Newtonian particles
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This equation can be rearranged to obtain the conventional statement
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The term momentum is the modern English word used for translating the phrase; quantity of motion.1Isaac Newton, Mathematical Principles of Natural Philosophy, page 639. Translated by Andrew Motte and Florian Cajori. University of California Press, 1934. So the foregoing relationship was articulated by Sir Isaac Newton when he wrote2Isaac Newton, Mathematical Principles of Natural Philosophy, page 404. Translated by I. Bernard Cohen and Anne Whitman. University of California Press, 1999.
Quantity of motion is a measure of motion that arises from the velocity and the quantity of matter jointly.
— Sir Isaac Newton
This direct proportionality between speed and momentum is traditional and simple. It can be used to eliminate the momentum in some previously defined quantities such as the Lorentz factor
which can now be expressed as

And for Newtonian particles the kinetic energy can be written as
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Momentum
Old discussion of Momentum
Momentum is the modern English word used for translating the phrase “quantity of motion” that Sir Isaac Newton uses on the very first page of his great book, the Principia3Isaac Newton, Mathematical Principles of Natural Philosophy, page 639. Translated by A Motte and F Cajori. University of California Press, 1934.. So to understand motion EthnoPhysics starts by using sensation to define the momentum as follows.
Consider some particle P characterized by its wavevector
and the total number of quarks it contains
Report on any changes relative to a frame of reference F which is characterized using
the average wavevector of the quarks in F. We define the momentum of particle P, in reference frame F, as the ordered set of three numbers
![]()
where
and
are constants.
The norm of the momentum is marked without an overline as ![]()
Momentum is traditionally understood as a product of the mass with a velocity. But the premise of EthnoPhysics questions how we accept spatial ideas like velocity. So instead we start with this sensation-based definition of momentum. Then later, after untangling some entwined concepts, we show how
for many particles and conditions.
Sensory Interpretation: The momentum is defined by a difference between the wavevector of P and a scaled-down version of the frame’s wavevector. Recall that the wavevector has previously been interpreted as a mathematical representation of lateral and visual sensation. So momentum is like the audio-visual contrast between a particle and its reference frame. This juxtaposition attracts and holds our attention because it is necessary for situational awareness and survival. The EthnoPhysics definition of momentum works by expressing the relevance of reference sensations. Seeing the Sun, seeing blood and seeing gold are vividly pertinent for understanding motivation, movement and motion.
Momentum is Conserved
Recall that quarks are conserved. So if some particles
,
and
interact like
but are otherwise isolated, then
the total number of quarks, is constrained as
Also, as shown earlier, wavevectors are combined as
if these particles are free. Then by substitution into the definition of momentum
![Rendered by QuickLaTeX.com \begin{align*} \overline{p}^{\,\mathbb{Z}} &\equiv \dfrac{h}{2\pi} \left[ \overline{\kappa}^{\,\mathbb{Z}} \! - N^{\mathbb{Z}}_{\mathsf{q}} \, \widetilde{\kappa}^{\,\mathsf{F}} \right] \\ &= \rule{0px}{15px}\dfrac{h}{2\pi} \left[ \left( \overline{\kappa}^{\mathbb{X}} + \overline{\kappa}^{\mathbb{Y}} \right) - \left( N_{\mathsf{q}}^{\mathbb{X}} + N_{\mathsf{q}}^{\mathbb{Y}} \right) \widetilde{\kappa}^{\,\mathsf{F}} \rule{0px}{15px} \right] \\ &= \dfrac{h}{2\pi} \left[ \left( \overline{\kappa}^{\,\mathbb{X}} \! - N^{\mathbb{X}}_{\mathsf{q}} \, \widetilde{\kappa}^{\,\mathsf{F}} \right) + \left( \overline{\kappa}^{\,\mathbb{Y}} \! - N^{\mathbb{Y}}_{\mathsf{q}} \, \widetilde{\kappa}^{\,\mathsf{F}} \right) \rule{0px}{15px} \right] \\ &= \rule{0px}{15px} \dfrac{h}{2\pi} \left( \overline{\kappa}^{\,\mathbb{X}} \! - N^{\mathbb{X}}_{\mathsf{q}} \, \widetilde{\kappa}^{\,\mathsf{F}} \right) + \dfrac{h}{2\pi} \left( \overline{\kappa}^{\,\mathbb{Y}} \! - N^{\mathbb{Y}}_{\mathsf{q}} \, \widetilde{\kappa}^{\,\mathsf{F}} \right) \\ &= \rule{0px}{15px} \; \overline{p}^{\mathbb{X}} + \overline{p}^{\mathbb{Y}} \end{align*}](https://www.ethnophysics.org/wp-content/ql-cache/quicklatex.com-e3579e87a8ab2097a866fcca97847d43_l3.png)
Thus we say that momentum is conserved when compound quarks are formed or decomposed. Newtonian mechanics is built on this relationship. It is important but not unique. Recall that we also have conservation laws for seeds, quarks, charge, lepton number, baryon number and enthalpy. All of these conservation rules follow from the logical requirements of our descriptive method. EthnoPhysics depends on mathematics. Therefore we are constrained by the law of noncontradiction and the associative properties of addition. So any characteristic defined by simple sums of quark coefficients will always be conserved.
Definition of Momentum
![]()
where
is called the direction of motion of P when presented in a Cartesian frame of reference. It is identified with the central-axis of P, written as
in quark-space. And it is completely arbitrary except for being a unit-vector.
De Broglie’s Postulate
In a perfectly inertial frame of reference
. Then the momentum of P is given by
![]()
And recall that for particles in motion, the wavelength is
. So taking the norm of the momentum and eliminating the wavenumber obtains Louis de Broglie’s statement about the inverse relationship between momentum and wavelength
![]()
Thus de Broglie’s postulate notes a conditional proportionality between
and
that is just built-in to the EthnoPhysics definitions of these characteristics. Moreover these definitions apply to all sorts of particles, photons as well as Newtonian particles. So De Broglie’s postulate is often used to determine the momentum of a photon since photons are usually described by their wavelength.
Momentum of a Graviton
Gravitons have been defined by the union of a photon and its associated anti-photon. This is written as
Also, recall that the wavevector
is defined from sums of quark coefficients, and that quarks are conserved. So the wavevector of a graviton is the sum of the wavevectors of its component photons. But the wavevector of any particle is symmetrically opposed to the wavevector of its matching anti-particle. Thus

Then, in a frame of reference noted by F, the momentum of a graviton is given by
![]()
where
is the total number of quarks in
including all types. This expression shows that all of the gravitons in a description have their momenta pointed in the same direction, and this direction is determined by attributes of the reference frame.
Acceleration
Consider a particle P described by a repetitive chain
of historically ordered space-time events
Let these events be characterized by their position
and time of occurrence
We express this trajectory of P by writing
![]()
Use these characteristics to calculate a velocity
for each event
Then changes between some arbitrary initial and final events are noted by
![]()
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The acceleration vector is defined by the ordered set of three numbers
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This acceleration is used to describe changes in the trajectory of P. It can be experimentally determined by measuring lengths and elapsed times. The norm of the acceleration is written without an overline
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Force and Newton’s Second Law
Consider a particle P described by a repetitive chain
of historically ordered space-time events
Let these events be characterized by their position
and time of occurrence
We represent this trajectory of P with the expression
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These characteristics may be used to establish the momentum
for each event
Then let P interact with some particle called
between initial and final events so that there is a change in P’s motion described by
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According to the usual narrative of Newtonian mechanics, the particle
impresses a force like a push or a pull that causes the change in P’s motion. Sir Isaac Newton says that4Isaac Newton, Mathematical Principles of Natural Philosophy, page 416. Translated by I. Bernard Cohen and Anne Whitman. University of California Press 1999.



— Sir Isaac Newton
This relationship is called Newton’s second law of motion. It can be mathematically expressed by defining an algebraic vector called the force as
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If P is a Newtonian particle in dynamic equilibrium, then its momentum is related to its velocity by
where
is its mass. Also for many sorts of interactions the mass of a Newtonian particle can be considered constant, then
and the force can be written in terms of the acceleration
as
![]()
Momentum is conserved. So all particles that have momentum can cause changes in the momentum of another particle if they are absorbed or emitted. Then X, the particle that is absorbed or emitted, is often called a force-carrying exchange particle.
Exchange particles that are material or charged are usually easy to detect in the immediate vicinity of an interaction. So the forces they impart are called contact forces. Phenomena like automobile collisions and gunshot wounds can be understood using contact forces. X is much less conspicuous if it is ethereal and neutral. Such particles can be difficult to detect, and the forces that they carry may seem to come from far away.
If X is imaginary then its force may seem like some random background fluctuation coming from nowhere specific. Many of these exchange particles are difficult to characterize and distinguish as individuals, so it is often more convenient to group lots of them together and refer to them collectively as force fields. For example we may vaguely refer to a set of photons as an electromagnetic field, or a collection of gravitons as a gravitational field.


Construction Zone
Types of Forces
Preparations for completing this discussion can be seen here: fields and forces
Centripetal Force
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For circular motion (as established by a choice for the spatial displacement vector) the magnitude of the centripetal force is a constant.
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From definitions of velocity and acceleration for circular motion
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Magnetic Force
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Observed as force on a current carrying wire.
Electric Force
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Observed as force in uniform field between capacitor plates.
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Coulomb Force
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Exchange particle: Coulomb force due to an interaction with a Coulomb photon formed by some field quanta from the ground-state of hydrogen which include electronic and muonic quarks .
Observed as: Coulomb’s law
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Gravitational Force
![]()
Exchange particle: Let
be due to an interaction with a graviton
only.
Observed as 1) Classroom field
![]()
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Observed as 2) Planetary field
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Strong Force
Exchange particle: strong force quanta
Observed as: transitions between energy levels of hydrogen


First Law of Motion
Consider a particle P described by a repetitive chain
of historically ordered space-time events
Let these events be characterized by their position
and time of occurrence
We express this trajectory of P by writing
![]()
These characteristics may be used to establish the momentum
for each event
By the second law of motion, any change in the momentum of P is related to the action of some force
that is described by
![]()
So if there are no forces acting on P, then there are also no changes in P’s momentum, and vice versa
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The forgoing statement is just a special case of the second law of motion. Yet Newton included this null relationship as part of his first law of motion. It may seem redundant, but the first law is more than simply a special case of the second law because it also establishes exactly what is meant by a straight line segment or a straight rod. The first law is also known as the law of inertia, it has been translated5Isaac Newton, Mathematical Principles of Natural Philosophy, page 416. Translated by I. Bernard Cohen and Anne Whitman. University of California Press 1999. into modern English as



— Sir Isaac Newton
For EthnoPhysics this first law is uniquely important because by our premise we prefer to avoid mysteriously received knowledge about length and lines. So this aspect of Newton’s first law is formally restated in the following explicit definition: If P has the same momentum for all events in its trajectory, then
describes uniform linear motion and we say that P is moving in a straight line. This sort of force-free motion is obtained if the frame of reference is inertial and P is isolated It is only well-defined for particles that are at least as big as atoms.
Collisions and Explosions
Here is an archetypal vignette from Newtonian mechanics. Two atoms called
and
have an interaction with each other by swapping another particle,
, which is called the exchange particle. The interaction is caused when
emits
at event
which is called the initial event of the interaction. This is written as
![]()
Particle
then has an effect on
by being absorbed at event
which is called the final event of the interaction. We express this by writing
![]()
For EthnoPhysics, the interaction is described using three repetitive chains of historically ordered events written as
![]()
![]()
![]()
Since
and
are composed from atoms, we assume that they can be described by space-time events with a position
and time of occurrence
. We do not assume that
is an atom, rather we often take it to be a photon or a graviton. So we cannot always describe
using a trajectory. And the position of
is well-defined only for the initial and final events where it is included as part of an atom. Overall, the interaction is characterized by the following quantities.
Momentum Change by Emission
The interaction is caused when
emits
at an event
which is called the initial event of the interaction. We write
But momentum is conserved so a total over all momenta
are the same before and after the interaction
![]()
Then the change in
‘s momentum due to the emission of
is given by
![]()
Momentum Change by Absorption
Particle
has an effect on
by being absorbed at event
which is called the final event of the interaction. We write
But momentum is conserved so a total over all momenta
are the same before and after the interaction
![]()
Then the change in
‘s momentum due to the emission of
is given by
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Karma and Newton’s Third Law
The third law of motion from Sir Isaac Newton is about a balance between the forces of cause and effect. It has been translated6Isaac Newton, Mathematical Principles of Natural Philosophy, page 417. Translated by I. Bernard Cohen and Anne Whitman. University of California Press, 1999. as



— Sir Isaac Newton
This has something in common with the ancient Indian idea of karma a key concept in Hindu, Jain, Buddhist, Tao, Shinto and Sikh philosophies. It is also similar to Western aphorisms like, ‘what goes around comes around’. And we suppose that Newton himself was well aware of passages in the Jewish and Christian texts about reaping and sowing.
But Newton’s third law is much more than just a vague claim of cosmic balance. It has a scientifically precise expression in terms of two atoms called
and
that have an interaction with each other by exchanging a third particle called ![]()
The interaction begins when
emits
As discussed earlier, the momentum change due to this event is given by
The emission causes the effect of
being absorbed into
. The momentum change due to absorption is
The elapsed time between emission and absorption is noted by
. The forces acting on
and
are found by substituting their momentum changes into the definition of force to obtain
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so the force of the cause is of equal size and in the opposite direction to the force of the effect.
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Thus Newton succeeded in articulating a wisp of widespread karmic wisdom. His approach leads to the enormous benefit of being susceptible of scientific investigation. Its range and accuracy can be tested in our laboratories. This process of measuring and checking is what makes Newtonian mechanics so trustworthy.


Experimental tests of Ethnophysics are discussed. Magnetic susceptibility and magnetic moments are defined and compared with observations.
| 1 | Isaac Newton, Mathematical Principles of Natural Philosophy, page 639. Translated by Andrew Motte and Florian Cajori. University of California Press, 1934. |
|---|---|
| 2 | Isaac Newton, Mathematical Principles of Natural Philosophy, page 404. Translated by I. Bernard Cohen and Anne Whitman. University of California Press, 1999. |
| 3 | Isaac Newton, Mathematical Principles of Natural Philosophy, page 639. Translated by A Motte and F Cajori. University of California Press, 1934. |
| 4, 5 | Isaac Newton, Mathematical Principles of Natural Philosophy, page 416. Translated by I. Bernard Cohen and Anne Whitman. University of California Press 1999. |
| 6 | Isaac Newton, Mathematical Principles of Natural Philosophy, page 417. Translated by I. Bernard Cohen and Anne Whitman. University of California Press, 1999. |


