# A geometrical meaning to the electron mass from breakdown of Lorentz invariance

**ABSTRACT** We discuss the problem of the electron mass in the framework of Deformed Special Relativity (DSR), a generalization of Special Relativity based on a deformed Minkowski space (i.e. a four-dimensional space-time with metric coefficients depending on the energy). We show that, by such a formalism, it is possible to derive the value of the electron mass from the space-time geometry via the experimental knowledge of the parameter of local Lorentz invariance breakdown, and of the Minkowskian threshold energy $E_{0,em}$ for the electromagnetic interaction. We put forward the suggestion that mass generation can be related, in DSR, to the possible dependence of mass on the metric background (relativity of mass).

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**ABSTRACT:**We illustrate the main features of a new Kaluza-Klein-like scheme (Deformed Relativity in five dimensions). It is based on a five-dimensional Riemannian space in which the four-dimensional space-time metric is deformed (i.e. it depends on the energy) and energy plays the role of the fifth dimension. We review the solutions of the five-dimensional Einstein equations in vacuum and the geodetic equations in some cases of physical relevance. The Killing symmetries of the theory for the energy-dependent metrics corresponding to the four fundamental interactions (electromagnetic, weak, strong and gravitational) are discussed for the first time. Possible developments of the formalism are also briefly outlined.06/2005;

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1

Fabio Cardone1,2, Alessio Marrani3 and Roberto Mignani2-5

1 Dipartimento di Fisica, Università dell'Aquila,

Via Vetoio

I - 67010 COPPITO,L'Aquila, Italy

2 I.N.D.A.M. - G.N.F.M.

3 Università degli Studi ''Roma Tre''

Via della Vasca Navale, 84

I-00146 ROMA, Italy

4 I.N.F.N. - Sezione di Roma III

5 mignani@fis.uniroma3.it

A geometrical meaning to the electron mass from breakdown of

Lorentz invariance

Abstract

We discuss the problem of the electron mass in the framework of Deformed Special

Relativity (DSR), a generalization of Special Relativity based on a deformed Minkowski

space (i.e. a four-dimensional space-time with metric coefficients depending on the

energy). We show that, by such a formalism, it is possible to derive the value of the

electron mass from the space-time geometry via the experimental knowledge of the

parameter of local Lorentz invariance breakdown, and of the Minkowskian threshold

energy E0,e.m. for the electromagnetic interaction. We put forward the suggestion that mass

generation can be related, in DSR, to the possible dependence of mass on the metric

background (relativity of mass).

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2

1 - Introduction

The problem of the mass spectrum of the known particles (leptons and hadrons) is

still an open one from the theoretical side. As a matter of fact, the Standard Model of

electromagnetic, weak and strong interactions is unable to say why a given particle does

bear that given (experimental) mass. As to the carriers of the four fundamental forces,

symmetry considerations would require they are all massless. However, it is well known

that things are not so simple: weak quanta are massive. It is therefore necessary, in the

framework of the Glashow-Weinberg-Salam model of electroweak interaction, to

hypothesize the Goldstone mechanism, able to give weak bosons a mass by interaction

with the (till now unobserved!) Higgs boson.

On this respect, even the first, best known and familiar particle, the electron, is still

a mysterious object. In spite of the successes of the Dirac equation, which allows one to

The origin of its mass is far from being understood. The classical electron theory (with the

works by Abraham, Lorentz and Poincaré) attempts at considering the mass of the electron

as of purely electromagnetic origin, and is well known to be deficient on several respects.

The basic flaw of such a picture is due to the Ernshaw theorem, stating that it is

impossible to have a stationary nonneutral charge distribution held together by purely

electric forces. Moreover, a purely electromagnetic model of the electron implies the

occurrence of divergent quantities. Such infinities can be dealt with by means of the

renormalization procedure in Quantum Electrodynamics (QED). However, even in this

framework, the value of the electron mass is not the intrinsic one but only that resulting

from its interaction with the vacuum.

The modern view to the problem of the electron mass is that pioneered by Wheeler

and Feynman(1), according to which it is not of electromagnetic origin but entirely

mechanical(2).

In this paper, we want to show that the electron mass me can be obtained from

arguments related to the breakdown of local Lorentz invariance, in the framework of a

generalization of Special Relativity ( Deformed Special Relativity, DSR), based on a

“deformation” of the Minkowski space (i.e. with metric coefficients depending on the

energy) . This allows one to attribute to me a geometrical meaning, by expressing it in

terms of the parameter d of LLI breakdown.

The organization of the paper is as follows. In Sect. 2 we briefly introduce the

concept of deformed Minkowski space, and give the explicit forms of the

phenomenological energy-dependent metrics for the four fundamental interactions. The

LLI breaking parameter dint for a given interaction is introduced in Sect. 3. In Sect. 4 we

assume the existence of a stable fundamental particle interacting gravitationally,

electromagnetically and weakly, and show (by imposing some physical requirements) that

its mass value (expressed in terms of de.m. and E0,grav is just the electron mass. In Sect. 5 we

briefly introduce the concept of mass relativity in DSR. Sect. 6 concludes the paper.

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3

2- Deformed Special Relativity in four dimensions (DSR)

2.1 - Deformed Minkowski space-time

Deformed Special Relativity is a generalization of Special Relativity (SR) based

on a ''deformed'' Minkowski space, assumed to be endowed with a metric whose

coefficients depend on the energy of the process considered(3). Such a deformation is

essentially aimed at providing a metric representation of the interaction ruling the process

considered (at least in the related energy range, and locally, i.e. in a suitable space-time

region)(3-6). DSR applies in principle to all four interactions (electromagnetic, weak, strong

and gravitational), at least as far as their non-local behavior and non-potential part are

concerned.

The generalized ("deformed'') Minkowski space

with the same local coordinates x of M4 (the four-vectors of the usual Minkowski space),

but with metric given by the metric tensor 1

(

[

)()()(

221100

EbEbEb

mmmm n

dddd

−−−≡

(

∈∀

0

RE

, where the {bµ2(E)} are dimensionless, real, positive functions of the energy(3).

The generalized interval in

4

M is therefore given by (xµ=(x0,x1,x2,x3)=(ct,x,y,z), with c

being the usual light speed in vacuum) (ESC on)

(

.)(

dxdxdxdxE

∗≡=

mn

h

The last step in (2.2) defines the scalar product ∗ in the deformed Minkowski

space

4

M 2. It follows immediately that it can be regarded as a particular case of a

Riemann space with null curvature.

Let us stress that, in this formalism, the energy E is to be understood as the energy

of a physical process measured by the detectors via their electromagnetic interaction in the

usual Minkowski space. Moreover, E is to be considered as a dynamical variable, because

1 In the following, we shall employ the notation "ESC on" ( "ESC off" ) to mean that the Einstein sum

convention on repeated indices is (is not) used.

2 Notice that our formalism - in spite of the use of the word ''deformation'' - has nothing to do with the

''deformation'' of the Poincaré algebra introduced in the framework of quantum group theory (in particular

the so-called k-deformations)(7). In fact, the quantum group deformation is essentially a modification of the

commutation relations of the Poincaré generators, whereas in the DSR framework the deformation concerns

the metrical structure of the space-time (although the Poincaré algebra is affected, too(8),(26)-(28)).

4

~

M (DMS4) is defined as a space

)

(

] )

)( ),( ),( ),()(

2

33

222

2

3

d

2

2

2

1

2

0

Eb

EbEbEbEbdiagE

ESCoff

≡

m

m n

h

−−−=

(2.1)

)

+

~

)

)()()()(

22

3

22

2

22

1

222

0

2

dzEbdyEbdxEbdtcEbds

=++−=

nm

(2.2)

~

Page 4

4

it specifies the dynamical behavior of the process under consideration, and, via the metric

coefficients, it provides us with a dynamical map - in the energy range of interest - of the

interaction ruling the given process. Let's recall that the use of momentum components as

dynamical variables on the same foot of the space-time ones can be traced back to

Ingraham(9) . Dirac(10), Hoyle and Narlikar(11) and Canuto et al.(12) treated mass as a

dynamical variable in the context of scale-invariant theories of gravity.

Moreover, it was shown that the DSR formalism is actually a five-dimensional

one, in the sense that the deformed Minkowski space can be naturally embedded in a

larger Riemannian manifold, with energy as fifth dimension(13) . Curved 5-d. spaces have

been considered by several Authors(14). On this respect, the DSR formalism is a kind of

generalized (non-compactified) Kaluza-Klein theory, and resembles, in some aspects, the

so-called ''Space-Time-Mass'' (STM) theory (in which the fifth dimension is the rest

mass), proposed by Wesson(15) and studied in detail by a number of Authors(16).

By putting ds2=0 , we get the maximal causal velocity in

≡

()(

21

EbEb

(i.e. the analogous of the light speed in SR) for the interaction represented by the

deformed metric considered.

In DSR the relativistic energy, for a particle of mass m subjected to a given

interaction and moving along

4

~

M

(3,21)

)(

)(

,

)

)(

,

)(

)(

3

000

Eb

Eb

c

Eb

c

Eb

cEur

(2.3)

ix ˆ ,has the form(3):

)(

~

g

)(

)(

)(

~

g

)(

2

0

2

22

E

Eb

Eb

cmEEumE

i

i

===

(2.4)

where ui is the i-th component of the maximal velocity (2.3) of the interaction considered,

and

(

1

)

i

i

i

ii

i

u

v

Ecb

Ebv

E

≡

−=−≡

−

−

b

bg

~

;

)(

)(

1

~

)(

~

2

1

2

0

2

1

2

(2.5)

In the non-relativistic (NR) limit of DSR, i.e. at energies such that

vi ÷ ui(E)

(2.6)

Eq. (2.4) yields the following NR expression of the energy corresponding to the given

interaction:

Page 5

5

(2.7)

2.2 - Energy-dependent phenomenological metrics

for the four interactions

As far as phenomenology is concerned, we recall that a local breakdown of

Lorentz invariance may be envisaged for all four fundamental interactions

(electromagnetic, weak, strong and gravitational) whereby one gets evidence for a

departure of the space-time metric from the Minkowskian one (at least in the energy

range examined). The experimental data analyzed were those of the following four

physical processes: the lifetime of the (weakly decaying) K0S meson(17); the Bose-Einstein

correlation in (strong) pion production(18); the superluminal photon tunneling(19); the

comparison of clock rates in the gravitational field of Earth(20). A detailed derivation and

discussion of the energy-dependent phenomenological metrics for all the four interactions

can be found in Ref.s [3-6]. Here, we confine ourselves to recall their following basic

features:

1) Both the electromagnetic and the weak metric show the same functional

behavior, namely

(

( ),( ),( , 1)(

EbEbEbdiagE

−−−=

m n

h

), )

222

(2.8)

()

0,1)(1

, 1

0,/

)(

3

1

0

0

0

0

3/1

0

2

>

−

−+=

=

<

≤<

E

=

E

E

E

EE

E

EEEE

Eb

q

(2.9)

(where ?(x) is the Heaviside theta function) with the only difference between them being

the threshold energy E0, i.e. the energy value at which the metric parameters are constant,

i.e. the metric becomes Minkowskian ( ?µ?(E= E0) = gµ? = diag(1,-1,-1,-1)); the fits to the

experimental data yield

E0,e.m. = (4.5± 0.2) µeV;

(2.10)

E0,weak =(80.4± 0.2) GeV;

)(

)(

)(

2

0

2

22

Eb

Eb

mcEmuE

i

i

NR

==

Page 6

6

Notice that for either interaction the metric is isochronous, spatially isotropic and ''sub-

Minkowskian'', i.e. it approaches the Minkowskian limit from below (for E<E0). Both

metrics are therefore Minkowskian for E>E0,weak > 80 GeV, and then our formalism is

fully consistent with electroweak unification, which occurs at an energy scale ~ 100 GeV.

Let us recall that the phenomenological electromagnetic metric (2.8)-(2.10) was

derived by analyzing the propagation of evanescent waves in undersized waveguides(17). It

allows one to account for the observed superluminal group speed in terms of a nonlocal

behavior of the waveguide, just described by an effective deformation of space-time in its

reduced part(5). As to the weak metric, it was obtained by fitting the data on the meanlife

of the meson K0S (experimentally known in a wide energy range (30÷350 GeV)(17)), thus

accounting for its apparent departure from a purely Lorentzian behavior(3,21).

2) For the strong interaction, the metric was derived(4) by analyzing the

phenomenon of Bose-Einstein (BE) correlation for p -mesons produced in high-energy

hadronic collisions(18). Such an approach permits to describe the BE effect as the decay of

a ''fireball'' whose lifetime and space sizes are directly related to the metric coefficients

b2µ,strong(E), and to avoid the introduction of ''ad hoc'' parameters in the pion correlation

function(4). The strong metric reads

(

),( ),()(

, 1 , 0

EbEb diagE

strongstrongstrong

−=

h

E

) )(),(

2

, 3

2

, 2

22

EbEb

strongstrong

−−

(2.11)

()

0,1)(1

,/

0, 1

E

)()(

, 0

5

2

)(

5

2

)(

2

, 0

, 0

, 0

2

, 0

, 0

<

2

, 3

2

, 0

2

2

, 2

2

2

, 1

b

>

−

−+=

=

≤<

E

==

>∀

=

=

E

E

E

EE

EE

EE

EbEb

Eb

E

strong

strong

strongstrong

strong

strongstrong

strong

strong

q

(2.12)

with

E0,strong = ( 367.5± 0.4) GeV . (2.13)

a deformation of the time coordinate occurs; moreover, the three-space is anisotropic,

with two spatial parameters constant (but different in value) and the third one variable

with energy like the time one.

Let us stress that, in this case, contrarily to the electromagnetic and the weak ones,

Page 7

7

experimental data on the relative rates of clocks in the Earth gravitational field(20). Its

explicit form is3:

(

),(),()(

, 1 , 0

EbEb diagE

gravgrav grav

−−=

h

, 1

3) The gravitational energy-dependent metric was obtained(6) by fitting the

) )( ),(

2

, 3

2

, 2

22

EbEb

grav grav

−

(2.14)

0,11

4

1

)(1

,1

4

1

0

)()(

2

, 0

, 0

, 0

2

, 0

, 0

2

, 3

2

, 0

>

−

+−+=

=

<

+

≤<

==

E

E

E

EE

EE

E

E

EE

EbEb

grav

grav

grav

grav

grav

grav grav

q

(2.15)

with

E0,grav = (20.2± 0.1) µeV . (2.16)

Intriguingly enough, this is approximately of the same order of magnitude of the thermal

energy corresponding to the 2.7°K cosmic background radiation in the Universe4.

Notice that the strong and the gravitational metrics are over-Minkowskian (namely,

they approach the Minkowskian limit from above (E0<E), at least for their coefficients

b02(E) = b32(E)).

3 - LLI breaking factor in DSR

The breakdown of standard local Lorentz invariance (LLI) is expressed by the LLI

breaking factor parameter d (23). We recall that two different kinds of LLI violation

parameters exist: the isotropic (essentially obtained by means of experiments based on the

propagation of e.m. waves, e.g. of the Michelson-Morley type), and the anisotropic ones

(obtained by experiments of the Hughes-Drever type(23), which test the isotropy of the

nuclear levels).

In the former case, the LLI violation parameter reads(23)

3 The coefficients b2

4 It is worth stressing that the energy-dependent gravitational metric (2.14)-(2.16) is to be regarded as a local

representation of gravitation, because the experiments considered took place in a neighborhood of Earth, and

therefore at a small scale with respect to the usual ranges of gravity (although a large one with respect to the

human scale).

1,grav(E) and b2

2,grav(E) are presently undetermined at phenomenological level.

Page 8

8

vcu

c

+

u

=

−

=

, 1

2

d

(3.1)

where c is, as usual, the speed of light in vacuo, v is the LLI breakdown speed (e.g. the

speed of the preferred frame) and u is the new speed of light (i.e. the ''maximal causal

speed'' in Deformed Special Relativity(3)). In the anisotropic case, there are different

contributions dA to the anisotropy parameter from the different interactions. In the HD

experiment, it is A=S, HF, ES, W, meaning strong, hyperfine, electrostatic and weak,

respectively. These correspond to four parameters dS (due to the strong interaction), dES

(related to the nuclear electrostatic energy), dHF (coming from the hyperfine interaction

between the nuclear spins and the applied external magnetic field) and dW (the weak

interaction contribution).

All the above tests put upper limits on the value of d (23).

Moreover, at the end of the past century, a new electromagnetic experiment was

proposed(24), aimed at directly testing LLI. It is based on the possibility of detecting a non-

zero Lorentz force between the magnetic field B generated by a stationary current I

circulating in a closed loop γ, and a charge q, in the hypothesis that both q and γ are at rest

in the same inertial reference frame. Such a force is zero, according to the standard

(relativistic) electrodynamics. The results obtained by such a method in two experimental

runs(25) admit as the most natural interpretation the fact that local Lorentz invariance is

in.fact broken.

The value of the (isotropic) LLI breaking factor determined by this electromagnetic

experiment is(25)

d ≅ 4·10-11

and represents the present lowest limit to d.

In order to establish a connection with the electron mass, we can define the LLI

breakdown parameter for a given interaction, dint , as

mm

−

≡

d

(3.2)

. int,

.,

. int,

.,. int,

int

1

in

gravin

in

gravinin

m

m

m

−=

(3.3)

where min.,int. is the inertial mass of the particle considered with respect to the given

interaction5 . In other words, we assume that the local deformation of space-time

corresponding to the interaction considered, and described by the metric (2.1), gives rise

to a local violation of the Principle of Equivalence for interactions different from the

gravitational one. Such a departure, just expressed by the parameter dint, does constitute

also a measure of the amount of LLI breakdown. In the framework of DSR, dint embodies

5 Throughout the present work, ''int'' denotes a physically detectable fundamental interaction, which can be

operationally defined by means of a phenomenological energy-dependent metric of deformed-Minkowskian

type.

Page 9

9

the geometrical contribution to the inertial mass, thus discriminating between two

different metric structures of space-time.

Of course, if the interaction considered is the gravitational one, the Principle of

Equivalence strictly holds, i.e.

min.,grav.= mg

where mg is the gravitational mass of the physical object considered, i.e. it is its

''gravitational charge'' (namely its coupling constant to the gravitational field).

Then, we can rewrite (3.3) as:

mm

−==

d

(3.4)

. .,int

in

..,int

in

..,int

in

m

. int

1

gg

m

m

−

(3.5)

and therefore, when the particle is subjected only to gravitational interaction, it is

dgrav. = 0

In the case of the gravitational metric (2.14)-(2.15), we have

)(

Eb

grav

Therefore, for i=3 , Eq. (2.4) yields, for the gravitational energy of a particle moving along

the z-axis (v3=v):

(3.6)

+

∈∀=

0

., 3

. , 0

, 1

)(

RE

Eb

grav

(3.7)

,1

2

2

1

2

2

g

cm

c

v

cmE

gggrav

=

−=

−

(3.8)

with non-relativistic limit (cfr. Eq. (2.7))

(3.9)

namely, the gravitational energy takes its standard, special-relativistic values.

This means that the special characterization (corresponding to the choice i=3) of

Eq.s (2.4) and (2.7) within the framework of DSR relates the gravitational interaction with

SR, which is - as well known - based on the electromagnetic interaction in its

Minkowskian form.

2

,

cmE

gNRgrav

=

Page 10

10

4 - The electron as a fundamental particle and its ''geometrical'' mass

Let us consider for E the threshold energy of the gravitational interaction:

E = E0,grav

where E0,grav is the limit value under which the metric ?µ?,grav (E) becomes minkowskian

(at least in its known components). Indeed, from Eq.s (2.14), (2.15) it follows:

(

[

gravgrav

EbEb

, 22 , 110

)()(

−−−=

mmm m n

ddddd

Notice that at the energy E = E0,grav the electromagnetic metric (2.8),(2.9) is

Minkowskian, too (because E0,grav >E0,e.m.).

On the basis of the previous considerations, it seems reasonable to assume that the

physical object (particle) p with a rest energy (i.e. gravitational mass) just equal to the

threshold energy E0,grav , namely

E0,grav = mg,pc2

must play a fundamental role for either e.m. and gravitational interaction. We can e.g.

hypothesize that p corresponds to the lightest mass eigenstate which experiences both

force fields (i.e., from a quantum viewpoint, coupling to the respective interaction carriers,

the photon and the graviton). As a consequence, p must be intrinsically stable, due to the

impossibility of its decay in lighter mass eigenstates, even in the case such a particle is

subject to weak interaction, too (i.e. it couples to all gauge bosons of the Glashow-

Weinberg-Salam group SU(2) × U(1), not only to its electromagnetic charge sector).

Since, as we have seen, for E = E0,grav the electromagnetic metric is minkowskian,

too, it is natural to assume, for p:

min,p,e.m. = min,p

namely its inertial mass is that measured with respect to the electromagnetic metric.

Then, due to the Equivalence Principle (see Eq. (3.4)), the mass of p is

characterized by

=

pin

mm

,p,e.m.in,

(4.1)

)

]

(

, 0

)

grav

ESCoff

grav

, 2

gravgrav

EE

EbEb diagE

, 03

22

22

, 1

,

1 ),(),(, 1)(

∈∀

−−−=

m

h

(4.2)

(4.3)

(4.4)

=

pg

mm

p

,gravp,in,

:

(4.5)

Page 11

11

interaction becomes:

Therefore, for such a fundamental particle the LLI breaking factor (3.3) of the e.m.

()

..,,

.,

.,

.,

,.,

..

1

1

mepinpg

p in

pg

p in

pgp

m

in

me

mm

m

mmm

d

d

−=⇔

−=

−

≡

(4.6)

Replacing (4.3) in (4.6) yields:

()

..

2

, 0

c

,

2

.., , 0

1

1

d

1

me

grav

pinmepingrav

E

mcmE

d

−

=⇔−=

(4.7)

Eq. (4.7) allows us to evaluate the inertial mass of p from the knowledge of the

electromagnetic LLI breaking parameter de.m. and of the threshold energy E0,grav of the

gravitational metric.

On account of Eq. (3.1), we can relate the lowest limit to the LLI breaking factor

of electromagnetic interaction, Eq. (3.3) (determined by the coil-charge experiment), with

de.m as follows:

d =1 - de.m. ≅ 4·10-11

Then, inserting the value (2.16) for E0,grav 6 and (4.8) in (4.7), we get

MeV

cc

..

1041

×−

d

(with min,e being the electron mass) where the ≥ is due to the fact that in general the LLI

breaking factor constitutes an upper limit (i.e. it sets the scale under which a violation of

LLI is expected). If experiment [25] does indeed provide evidence for a LLI breakdown

(as it seems the case, although further confirmation is needed), Eq. (4.9) yields min,p=min,e.

We find therefore the amazing result that the fundamental particle p is nothing but the

electron e- (or its antiparticle e+ 7). The electron is indeed the lightest massive lepton

(pointlike, non-composite particle) with electric charge, and therefore subjected to

gravitational, electromagnetic and weak interactions, but unable to weakly decay due to its

(4.8)

e in

me

grav

2

p in

m

c

eV

E

m

,

2211

−

5

, 0

,

5 . 0

1021

==

×

≥=

−

(4.9)

6 Let us recall that the value of E0,grav was determined by fitting the experimental data on the slowing down

of clocks in the Earth gravitational field (20) . See Ref. [6].

7 Of course, this last statement does strictly holds only if the CPT theorem maintains its validity in the DSR

framework, too. Although this problem has not yet been addressed in general on a formal basis, we can state

that it holds true in the case we considered, since we assumed that the energy value is E = E0,grav

corresponding to the Minkowskian form of both electromagnetic and gravitational metric.

Page 12

12

small mass. Consequently, e- (e+) shares all the properties we required for the particle p,

whereby it plays a fundamental role for gravitational and electromagnetic interactions.

5 – Mass relativity in DSR

the electron mass to the (local) breakdown of Lorentz invariance. Such a mass would then

be a measure of the deviation of metric from the Minkowskian one. The minimum

measured mass of a particle would be related to the minimum possible metric deviation

compatible with its interactions.

Such a point can be reinforced by the following argument.

physical standpoint, as the speed of the quanta of the interaction locally (and

phenomenologically) described in terms of a deformed Minkowski space. Since these

quanta are associated to lightlike world-lines in

(with respect to the interaction considered), in analogy with photons (with respect to the

e.m. interaction) in the usual SR.

Let us clarify the latter statement. The carriers of a given interaction propagating

with the speed ur typical of that interaction are actually expected to be strictly massless

only inside the space whose metric is determined by the interaction considered. A priori,

nothing forbids that such “deformed photons'' may acquire a non-vanishing mass in a

deformed Minkowski space related to a different interaction.

This might be the case of the massive bosons W+ , W- and Z0, carriers of the weak

interaction. They would therefore be massless in the space

weak interaction, but would acquire a mass when considered in the standard Minkowski

space M of SR (that, as already stressed, is strictly connected to the electromagnetic

interaction ruling the operation of the measuring devices). In this framework, therefore, it

is not necessary to postulate a ''symmetry breaking'' mechanism (like the Goldstone one in

gauge theories) to let particles acquire mass. On the contrary, if one could build up

measuring devices based on interactions different from the e.m. one, the photon might

acquire a mass with respect to such a non-electromagnetic background.

Mass itself would therefore assume a relative nature, related not only to the

interaction concerned, but also to the metric background where one measures the energy

of the physical system considered. This can be seen if one takes into account the fact that

in general, for relativistic particles, mass is the invariant norm of 4-momentum, and what

is usually measured is not the value of such an invariant, but of the related energy.

The considerations carried out in the previous Sections allow us therefore to relate

The maximal causal velocity ur defined by Eq. (2.3) can be interpreted, from a

4

~

M , they must be zero-mass particles

4

~

M (hweak(E)) related to the

Page 13

13

5 - Conclusions

The formalism of DSR describes -among the others -, in geometrical terms (via the

energy-dependent deformation of the Minkowski metric) the breakdown of Lorentz

invariance at local level (parametrized by the LLI breaking factor dint). We have shown

that within DSR it is possible - on the basis of simple and plausible assumptions - to

evaluate the inertial mass of the electron e- (and therefore of its antiparticle, the positron

e+) by exploiting the expression of the relativistic energy in the deformed Minkowski

space

+

∈0

RE

gravitational interaction (in particular its threshold energy), and the LLI breaking

parameter for the electromagnetic interaction de.m..

Therefore, the inertial properties of one of the fundamental constituents of matter

and of Universe do find a ''geometrical'' interpretation in the context of DSR, by admitting

for local violations of standard Lorentz invariance.

We have also put forward the idea of a relativity of mass, namely the possible

dependence of the mass of a particle on the metric background where mass measurements

are carried out. This could constitute a possible mechanism of mass generation alternative

to those based on symmetry breakdown in Relativistic Quantum Theory.

)(

~

M

4

E

, the explicit form of the phenomenological metric describing the

Page 14

14

References

1. J.A Wheeler and R. P. Feynman: Rev. Mod. Phys. 17, 157 (1945). ibidem, 21, 425

(1949).

2. M. H. Mac Gregor: The Enigmatic Electron (Kluwer, Dordrecht,1992).

3. F. Cardone and R. Mignani: ''On a nonlocal relativistic kinematics'', INFN preprint

n.910 (Roma, Nov. 1992); Grav. & Cosm. 4 , 311 (1998); Found. Phys. 29, 1735

(1999); Ann. Fond. L. de Broglie 25 , 165 (2000).

4. F. Cardone and R. Mignani: JETP 83, 435 [Zh. Eksp. Teor. Fiz.110}, 793] (1996); F.

Cardone, M. Gaspero, and R. Mignani: Eur. Phys. J. C 4, 705 (1998).

5. F.Cardone and R.Mignani: Ann. Fond. L. de Broglie, 23 , 173 (1998); F. Cardone, R.

Mignani, and V.S. Olkhovski: J. de Phys.I (France) 7, 1211 (1997); Modern Phys.

Lett. B 14, 109 (2000).

6. F. Cardone and R. Mignani: Int. J. Modern Phys. A 14, 3799 (1999).

7. See e.g. P. Kosinski and P. Maslanka, in ``From Field Theory to Quantum Groups'',

eds. B. Jancewicz, J.Sobczyk (World Scientific, 1996), p. 11; J. Lukierski, in Proc. of

Alushta Conference on Recent Problems in QFT, May 1996, ed. D. Shirkov, D.I.

Kazakov, and A.A. Vladimirov (Dubna 1996), p.82; J. Lukierski, ?-Deformations of

relativistic symmetries: recent developments, in Proc. of Quantum Group Symposium,

July 1996, Goslar, ed. H.-D. Doebner and V.K. Dobrev (Heron Press, Sofia, 1997), p.

173; and refs. therein.

8. F. Cardone, A. Marrani and R. Mignani: ''Killing symmetries of generalized

Minkowski spaces. 1- Algebraic-infinitesimal structure of space-time rotation groups'',

Found. Phys. 34, 617 (2004) ), hep-th/0505088.

9. R.L. Ingraham: Nuovo Cim. 9, 87 (1952).

10. P.A.M.Dirac: Proc. R. Soc. (London) A333, 403 (1973); ibidem, A338, 439 (1974).

11. F. Hoyle and J.V. Narlikar: ''Action at a Distance in Physics and Cosmology''

(Freeman, N.Y., 1974).

12. V.Canuto, P.J.Adams, S.-H.Hsieh and E.Tsiang: Phys. Rev. D16, 1643 (1977);

V.Canuto, S.-H.Hsieh and P.J.Adams: Phys. Rev. Lett. 39, 429 (1977).

13. F. Cardone, M. Francaviglia, and R. Mignani: Gen. Rel. Grav. 30, 1619 (1998);

ibidem, 31, 1049 (1999); Found. Phys. Lett. 12, 281, 347 (1999).

14. See V. G. Kadyshevsky, R. M. Mir-Kasimov and N. B. Skachkov: Yad. Fiz. 9, 212

(1969); V. G. Kadyshevsky: Nucl. Phys. B141, 477 (1978); V. G. Kadyshevsky, M. D.

Mateev, R. M. Mir-Kasimov and I. P. Volobuev: Theor. Math. Phys. 40, 800 (1979)

[Teor. Mat. Fiz. 40, 363 (1979)]; V. G. Kadyshevsky and M. D. Mateev: Phys. Lett. B

106, 139 (1981); Nuovo Cim. A 87, 324 (1985); A. D. Donkov, R. M. Ibadov, V. G.

Kadyshevsky, M. D. Mateev and M. V. Chizhov, ibid. 87, 350. 373 (1985); and

references therein.

15. P.S.Wesson: Astron. Astrophys. 119, 145 (1983); Gen. Rel. Grav. 16, 193 (1984).

16. See e.g. J.M.Overduin and P.S.Wesson: Phys. Rept. 283, 303 (1997), and references

therein.

17. S.H.Aronson, G.J.Bock, H.-Y.Chang and E.Fishbach : Phys. Rev. Lett. 48, 1306

(1982); Phys. Rev. D 28, 495 (1983); N.Grossman et al.: Phys. Rev. Lett. 59, 18

(1987).

Page 15

15

18. For experimental as well as theoretical reviews, see e.g. B.Lörstad: ''Correlations and

Multiparticle Production (CAMP)'', eds. M. Pluenner, S. Raha and R. M. Weiner

(World Scientific, Singapore, 1991); D.H. Boal, C.K. Gelbke and B. K. Jennings: Rev.

Mod. Phys. 62, 553 (1990); and references therein.

19. For reviews on both experimental and theoretical aspects of superluminal photon

tunneling, see e.g. G.Nimtz and W.Heimann:Progr. Quantum Electr. 21, 81 (1997);

R.Y.Chiao and A.M.Steinberg : ''Tunneling Times and Superluminality'', in Progress

in Optics, E.Wolf ed., 37, 346 (Elsevier Science, 1997); V.S.Olkovsky and A.Agresti:

in ''Tunneling and its Implications'', D.Mugnai, A.Ranfagni and L.S.Schulman

eds.(World Sci., Singapore, 1997), p.327.

20. C.O.Alley: ''Relativity and Clocks'', in Proc. of the 33rd Annual Symposium on

Frequency Control, Elec.Ind.Ass., Washington, D.C. (1979).

21. F. Cardone, R. Mignani and R. M. Santilli: J. Phys. G 18, L61, L141 (1992).

22. F. Cardone, A. Marrani and R. Mignani: ''Boosts in an arbitrary direction and maximal

causal velocities in a deformed Minkowski space'', Found. Phys. Lett. 16, 163 (2003)

), hep-th/0505032.

23. See C.M.Will: ''Theory and Experiment in Gravitational Physics'' (Cambridge

Univ.Press, rev.ed.1993), and references therein.

24. U. Bartocci and M. Mamone Capria: Am. J. Phys. 59, 1030 (1991); Found. Phys. 21,

787 (1991).

25. F.Cardone and R.Mignani: Physics Essays 13, 643 (2000); ''On possible experimental

evidence for a breakdown of local Lorentz invariance'' , in ''Gravitation,

Electromagnetism and Cosmology: Toward a New Synthesis'' (Proc. Int. Conf. On

Redshifts and Gravitation in a Relativistic Universe, Cesena, Italy, Sept. 17-20, 1999),

ed. by K. Rudnicki (Apeiron, Montreal, 2001), p. 165; U.Bartocci, F.Cardone and

R.Mignani: Found. Phys. Lett. 14, 51 (2001).

26. A. Marrani: ''Simmetrie di Killing di Spazi di Minkowski generalizzati'' (''Killing

Symmetries of Generalized Minkowski Spaces'') (Laurea Thesis), Rome, October 2001

(in Italian).

27. F. Cardone, A. Marrani and R. Mignani: ''Killing symmetries of generalized

Minkowski spaces. 2- Finite structure of space-time rotation groups in four

dimensions'', Found. Phys. 34, 1155 (2004) , hep-th/0505105.

28. F. Cardone, A. Marrani and R. Mignani: ''Killing symmetries of generalized

Minkowski spaces. 3- Space-time translations in four dimensions'', Found. Phys. 34,

1407 (2004), hep-th/0505116 .

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