Paragraph B12. Singularities
One writes any TU*[t^^] to be a function of 1/t^^ to change to finite the infinite t^^ = tlim^^ occuring in dt and the infinite t^^ = tl^^ occuring in D1. In par. B12(A1) it is argued lowest order terms are sufficient to describe TU*[t^^]. Any transformation TU can be reduced to Taylor series TU*[t^^] = 1 + Σn Yn. (1/t^^)^n, n=1 to n infinite, the Yn constants.
Consider the time interval version for transformation TU for time interval domain d∆t^^, i. e. TU*[∆t^^] = Σn Yn. Xn.
∆t^^i, n=1 to n infinite, the Taylor series linear in multiplication inverse ∆t^^i due to property eq. 1. The set generator approach for the time interval set gives the same result, par. B12(A4). Recall the time interval current parameter ∆w ~ w can be defined from the averages definition for correspondence or from the set units and zero’s, even though ∆w does not follow equilibrium time development. TU*[dw] for domain dw is defined in B12(A6).
For surface parts Pi(N, w, tlim^^), for N = 2 in example (PP), the two parameters w and tlim^^, or similarly the domains dw and dt, remain inter-dependent to assure the surface domain measure mdTU*I*[dw x dt] = m(dTU*I*[dw] x dTU* I*[dt]) remains invariant, which means TU*I equals a specific Lorentz transformation TS. This is valid for TU*I equal to the identity, trivially. Assumed is the diagonal metric for one moment time space time to simplify the measures. This choice is legitimate since, with specific Lorentz transformations TS, surface measure remains invariant, at least for the time interval description, due to which measures remain to fulfill the covering least requirement.
A1. Transformation TU for domain dt with transit parameter ε for singularity t0
With TU any transformation, TU[t^^] = 1 + Σn. Yn. (1/t^^)^n, n=1 to n infinite, with current parameter t^^ from domain dt, a singularity exists at t^^ = t0^^ = u0. Chosen is transformation TU*[t^^] = (1/t^^) for the example construction II, which seems universal due to the arguments in comment B8.
To resolve the singularity, domain dt = [t0^^, tlim^^], is written as an addition, assuming addition trivially can be applied to domain sets, considering comments B12 to B14. dt = dMt + dPt = [0, ε’] + [ε’, tlim^^], and similar for surface parts Pi indicated with M and P: Pi = PMi(N, w, tlim^^) + PPi(N, w, tlim^^), with dPMi = H[ε’]. dPi and dPPi = (1 - H[ε’]). dPi, with H[ε’] the usual Heaviside function with infinitesimal transition parameter t^^ = ε’. Transformation TU*[1/t^^] can be written with lowest, linear, terms only, comment B8.
Comment B8. There is an argument, where a solution of a functional equation, completely separable in say two variables, f(a + b) = f(a) + f(b), is ‘nearly always’ of linear form f(x) = m. x, with m constant and a, b, x the variables. The ‘nearly always’ implies ‘always’ when the solution is bounded over the two interval domains for a and b, (Hocking, Young, 1961). This is similar to the canonical property for f(x), x the variable, e. g. x = dq/dt, with q the generalized space like coordinate within the one moment time description. The canonical property mostly refers to multiplication rather than addition. It allows for the introduction of set or group generators for the functional f(x).
A linear terms approximation for TU is valid when separable domains dw and dt are assumed (Arnold, 1989). This can be applied when considering generators G, in terms of exponents f(x) = exp(x. G) for the solution set for functionals f(x), par. B12(A4), and already in (Hollestelle, 2020). Within the time interval only set there is exactly one generator, time interval ∆t, due to the multiplication linearity theorem (Hollestelle, 2024).
The second part, due to transition parameter ε’, for domain dt = [0, tlim^^], is dtP = [ε’, tlim^^], transformed to domain dTU[dtP] = [1/tlim^^, 1 – (1/ε’)]. When domain [ε’, t^^lim] is open, [1/tlim^^, 1 – (1/ε’)] is open similarly. The first part of dt is dtM = [0, ε’], transformed to dTU[dtM] = [1 – (1/ε’), tl^^] with tl^^ = ‘addition unit’||dt. Transition parameter ε’ is consistent with parameter ε = ε’, with r = 1/(1 + ε), par. B9 and eq. B10, including ε = tlim^^, derived in par. B12(A3), without loss of universality.
A2. Transformation I
Transformation I is introduced to interchange t^^ values t0 and tl, with dt = [t0^^, tlim^^], and for which I*[tl^^] = t0^^
<< I*[t0^^] = tl^^, with tl^^ outside dt since r = tlim^^/tl^^ < 1, solving the singularity problem of TU for t^^ = t0^^ in par. B12(A1) applying TU*I, when domain t^^ is defined with dt instead of D1 = [t0^^, tl^^].
Transformation I is followed by TU and one secures domain dI*[dt] = [I*[t0^^], I*[tlim^^]] = [tl^^, ε] = [ε, tl^^], with definition I*[tlim^^] = ε > I*[tl^^] = t0^^, for transit parameter ε from A1. Transformation I does not change parameter w from domain dw.
A3. Transformation I and the multiplication domain definition for current parameter t^^
For transformation I the inverse is I’, with I’*I*[w] = α. w with α invariant scalar. Scalar invariant α can be interpreted to scale domain dt = [t0, tlim], such that singularity I*[t0^^] = tl^^ is not within, rather outside dt, where transformation TU resembles inverse I’ for domain dt.
A complication is the dimensional domain definition of current parameter t^^. Any t^^ from D1 can be written t^^ = t^^[tv, tw] = tv. tw, with multiplication indication . and both tv and tw from D1. This is to solve the infinities occuring with the definition of t^^ within domain D1, due to the cardinal number of the specific scalar set S1, the set that includes the infinite values of tl^^ and tlim^^. This includes some intricate evaluation of the current parameter t^^ domain.
There is a difference in multiplication for t^^ finite and t^^ infinite. Meant is domain D1 = [t0^^, tl^^] includes two parts, the finite part with dt(finite) = [t0^^, tlim^^] and infinite part with dt(infinite) = [tlim^^, tl^^]. Eq. B13 is an expression for I*[t^^] when defining t^^ = t^^[tv, tw]. Indication v or w occurs for tv or tw, while indication letter l occurs for tl^^.
Comment B9. Inferred is: both tv and tw can be from dt(finite) or dt(infinite), however one from each domain, and t^^lim can be from both domains. Transformation I exchanges values to inverse values. Examples are given with eq. B13, where eq. B15 is the overall relation.
B13 I*[t^^] = I*[tv, tw] = (1/tv. tlim^^). (1/tw. tl^^)
t0^^ =I*[tl^^] = 1/tl^^. tlim^^, from dt(infinite) to dt(finite)
tl^^ = I*[t0^^] = tl^^. tlim^^. 1/tlim^^. tl^^, from dt(finite) to dt(infinite)
With ‘addition zero’||t^^ = ‘multiplication unit’||t^^ = tl^^ from dt(infinite), par. B8, and with tlim^^ from dt(finite) there is I*[tlim^^] = I*[tv = tl^^, tw = tlim^^] = (1/tl^^. tlim^^). (1/tlim^^. tl^^) = 1/tl^^. tl^^ = r. 1/tlim^^, belongs to dt(finite), while I*[tlim^^] = I*[tv = tlim^^, tw = tl^^] = tl^^, belongs to dt(infinite). This is consistent with eq. B14. One can define multiplication t^^ = [tv, tw] from domain dt(finite) and dt(infinite) to avoid contradiction.
B14 t^^ = t^^[tv: dt(finite), tw: dt(infinite)], remains in dt(infinite) t^^ = t^^[tv: dt(infinite), tw: dt(finite)], remains in dt(finite) tlim^^ = r. tl^^, remains in dt(infinite)
tlim^^ = tl^^. r, remains in dt(finite)
The multiplications can be applied for the definition of I for the one moment time version from correspondence with the time interval version. With transformation I applied to t^^ = tv. tw, the domain dt(finite) and dt(infinite) are exchanged. The special t^^ = tlim^^ can be from dt(finite) or dt(infinite). The time interval version units and zero’s can be derived due to eq. 1, meaning e. g. M[∆t3, ∆t] = M[∆t, ∆t3] = ∆t3 and M[∆t3, ∆t3] = ∆t3.
With the definition tl^^ = ‘multiplication unit’||t^^ for any current parameter t^^ from domain dt(finite) = [t0^^, tlim^^], there is t^^. tl^^ = t^^ remains in dt(infinite) and tl^^. t^^ = t^^ remains in dt(finite).
For any t^^ from domain dt(infinite) = [tlim^^, tl^^], with r = tlim^^/tl^^ < 1, there is tl^^. t^^ = t^^. tl^^ = t^^ in dt(infinite).
There is, even though multiplication not being well defined for t^^ from dt(infinite), however tl^^ = ‘multiplication unit’||t^^, and t^^ = tlim^^ in dt(infinite) implies tlim^^ = tlim^^. tl^^ remains in dt(infinite), while I*[tlim^^. tl^^] = tl^^. tl^^ >> I*[tl^^. tl^^] = t0^^ = 1/tl^^. tlim^^, as it should be.
Define within domain dt(finite), ε = 1/tlim^^ = 1/tlim^^. tlim^^, and 1/tlim^^ = tlim^^ = multiplication unit’||t^^, while within domain dt(infinite) defined is ε = 1/t0^^. tlim^^ = tl^^ = ‘multiplication unit’||t^^.
When t^^ = tlim^^ in dt(finite) and tlim^^ = tlim^^. tlim^^, there is I*[tlim^^. tlim^^] = 1/tlim^^ in dt(infinite). For dt(finite) =[t0^^, tlim^^], the following expression is consistent with t^^ = t^^[tv, tw] from eq. B13.
B15 I*[t^^] = 1/t^^. tlim^^
TU*I*[t^^] = TU*[1/t^^. tlim^^] = 1/(1/t^^. tlim^^) = t^^. 1/tlim^^ = t^^
A4. Time interval operators, the time interval multiplication ‘set rule’, and set generators
Theorem B3. from (Hollestelle, 2024). For set generators G and set elements t^^, and transformations T*(t^^) = exp[t^^. G], there is addition A equals multiplication M when set generators equal set elements, and this is precisely the case for the time interval only set.
One can apply generators for the one moment time set and for the time interval set. Group or set generators are widely and diversely applied, and introduced in e. g. (Veltman, 1974), (De Wit, Smith, 1986).
Comment B10. Where the usual one moment time description time parameter operator is a derivative, the definition for the corresponding time interval operator is from (Hollestelle, 2021): the time interval operator ‘working to the right’ on a quantity A1, not necessarily a time interval quantity, is defined with:
operator*[A1] = M[D*||∆t[|operator*|. A1], ∆t] = A[ |operator*|. D*||∆t[A1], D*||∆t[|operator*|] ].
The expression |operator*| indicates the operator quantity, D*||∆t[A1] is the time interval derivative of quantity A1, both occur in the time interval operator definition. The 2nd step is due to the time interval ‘set rule’ for the time interval derivative of multiplication for any time interval ∆t1 and any scalar a, derived in (Hollestelle, 2024):
D*||∆t[a. ∆t1] = A[a. D*||∆t[∆t1], D*||∆t[a] ]
for any, in this case time interval, quantity a. ∆t1. The one moment time ‘set rule’ provides usually the derivative definition for any one moment time quantity q1 and any scalar a:
d/dq*[a. q1] = c1. d/dq*[a]. q1 + c2. a. d/dq*[q1] = c2. a. d/dq*[q1]
The d/dq is the one moment time derivative, c1 and c2 are scalar constants dependent on the associative property, usually assumed is c1 = c2 = 1. Assumed is d/dq*[a] = ‘multiplication zero’||q for invariant scalar a, for the one moment time parameter q set.
Due to theorems 1b and 1c, par. 3.8, applied within the one moment time description, an equation in terms of scalar a with space like parameters can be changed to one in terms of time like parameters. One recognizes scalar a to ‘move to the left’ for both the one moment time description and the time interval description.
The Time Interval Version for Transformation TU*I
Within the time interval description, where the time interval only set is 1-dim. and the time interval generator is ∆G, defined is, for object ruler t^^ dependent on one moment time space like coordinate q: D*||∆q[∆t^^] = ∆αi and D*||
∆q[∆G] = ∆β, with ∆αi or ∆β not necessarily equal to ‘multiplication zero’||∆q. Apply the time interval ‘set rule’, while
∆A1 = ∆t^^ and scalar r = tlim^^/tl^^.
Theorem B5. The theorem on averages applies since α is measurement dependent, scale calibration dependent, when the derivative of current parameter w and t^^ to one moment time parameter t or time interval ∆t can be derived. When the current parameters, being object rulers, are assumed to follow equilibrium time development, they are simultaneous, and with their derivatives to ∆t equal to ‘multiplication zero’||∆t within the time interval description. This was discussed in par. 1.2, and assumes calibration of object ruler type of measuring ∆Pi and measuring wave propagation at surface ∆A.
Since the time interval set canonical property is valid, one can write, including only the 1st order derivatives, with time interval commutators [∆t, ∆t]||∆t = ∆t and [∆G, ∆G]||∆t = ∆G, where [∆t1, ∆t2]||∆t = M[ A[TS[∆t1], ∆t1i], ∆t2] = M[ I*||
∆t1 [∆t1], ∆t2] = ∆t2.
TU*I*[∆t^^] = exp[M[∆t^^, ∆G]] = exp[ M[ A[∆αi, ∆β], ∆G] ].
exp[ M[∆t^^, ∆G] ] = exp[ M[M[∆αi, ∆q], M[∆β, ∆q]] ] = exp[ M[∆αi, ∆G] ]
It follows ∆t^^ = M[∆t^^, ∆αi] where ∆αi = ∆t^^ and ∆β = ∆G. This implies D*||∆q[∆G] = ∆G, i. e. ∆G equals time interval Noether current ∆NC, considering ∆t = ∆q due to D||*∆t[∆q] = ‘multiplication unit’||∆t, par. 4.2.
Operator TU*I
From the ‘set rule’ applied to operator TU*I, one finds TU*I*[∆t^^] = A[ d1. ∆αi, D*||∆q[d1] ] with in this case d1 = | TU*I*| the operator TU*I quantity, a scalar since TU*I equals the identity.
One can define ∆M with exp[M[∆t^^, ∆G] ] = exp[∆M ], with a Taylor series. Multiplication of two time interval quantities M[∆t1, ∆t2] is again a time interval quantity, equal to say ∆t3, (Hollestelle, 2024), theorem 4. Not included in the original ‘set rule’ definition is time interval multiplication M[∆t1, ∆t2], rather scalar multiplication, however it is assumed applicable.
D*||∆q [M[∆t^^, ∆G] ] = M[∆t^^, ∆G] = ∆M
exp[∆M ] = 1 + (Σ(k ≥ 1) 1/k! ). M[∆M. exp[∆M] ] = A[(m – 1). M[∆M, exp[∆M] ]i, M[∆M, exp[∆M] ] = (m – 1). ∆t^^ Recall ∆M equals in this case ∆NC and ∆t^^, the ∆q dependent on the object ruler and ∆t^^, not on ∆t or equilibrium time development. Remains the following 1st order equations:
(m - 1). ∆t^^ = A[‘addition unit’||∆q, ∆M]. exp[ ∆M ] (m – 1). ∆t^^ = A[‘addition unit’||∆q, ∆M] = exp[ ∆M ]
(m – 1). ∆q = A[‘addition unit’||∆q, ∆M] = exp[∆t^^] = A[‘addition unit’||∆q, exp[ ‘addition zero’||∆q] ]
Trial solution is ∆αi = ∆α = ‘multiplication unit’||∆q = ∆q and it follows D*||∆q[∆q] = ∆q and ∆G = ∆q.
This is consistent with the operator result, D*||∆q[∆G] = ∆G, i. e. ∆G = ∆NC. It confirms the assumption that multiplication for two time interval quantities, within the time interval ‘set rule’, is applicable.
B17 TU*I*[∆t^^] = exp[ ∆M] = (m – 1). ∆t^^ = M[ M[‘addition unit’||∆q, ∆qi], ∆t^^] ] = ‘addition unit’||∆q = ∆t^^
The time interval transformation TU*I* is found to be equal to the time interval current parameter ∆t^^ identity operator, TU*I*[∆t^^] = ∆t^^. This is consistent with correspondence with one moment time current parameter results eq. B16, i. e. ∆t^^ ~ t^^, and TU*I*[t^^] = t^^. Recall the canonical property for the time interval only set is valid.
Correspondence can be derived from the units and zero’s, however the current parameter set for ∆t^^ or t^^ does not have to depend on ∆t or one moment time parameter t, and ∆t^^ ~ t^^ is not the same as ∆t ~ t.
Theorem B4. One can apply higher order approximations for TU*I*[∆t^^] in terms of the Taylor series in ∆t^^, to find the time interval version of TU*I*[∆t^^] = exp[ ∆M], applying eq. 1. Eq. B17 is universal for any operator TU*I, and both any time interval and one moment time description TU*I operator is equal to the identity operator.
Comment B12. Time interval operator TU*I*[∆t^^] allows space reversal symmetry, while time reversal symmetry is not allowed, ∆t^^ being related with ∆q = M[∆αi, ∆t^^] and where D*||∆t[∆q] = ∆t. To find TU*I*[∆t^^] from Kramers relation directly, par. 2.4, seems not feasible since ∆t and ∆t^^ are not related, assuming the current parameters remain independent of equilibrium time development. Some cases where however dependence can be assumed have been discussed in par. B8, e. g. ‘wave-group propagation collapse’ within ∆t, where the order of any wave function collapse can be interchanged.
A5. The combination TU*I and specific Lorentz transformations TS
The choice for TU leaves mdTU*[dt] invariant, since the specific Lorentz transformations TS, which are coordinate transformations for domain dw and dt, preserve surface measure at the propagation surface A, (Hollestelle, 2021). This means TS preserves quadratic measures at surface A, the metric being diagonal or non diagonal. It follows any TU transformation is a TS transformation. With eq. 18 it is assumed variables dw and dt can be separated, due to comment B13. Assumed is transformation I leaves dw invariant.
B18 dTU*I*[dw x dt] = dTU*[dw] x dTU*I*[t0, tlim]
B19 mdTU*I*[dw x dt] = mdTU*[dw]. mdTU*[tl, ε] = mdTU*[dw]. m[1/tl, 1/ε]
The x means 2-dim. outer-product in terms of surface part Pi dimensions d1 and d2, while trivialy domain [1, 0] equals domain [0, 1].
Comment B13. In terms of measures for dimensions d1 and d2 for Pi, assumed is measures mPi of the disjoint Pi can be added like scalar numbers to derive mPu.
Comment B14. Assumed is domain dq = |q|. dw for q = |q|. w, linear with any parameter q from any domain, including domain dw or domain dt.
Comment B15. Required is surface part TU*I*[Pi], for i = 1, 2, has to be disjoint, open and dense. However TU*I*[dw x dt] is always open when dw and dt open, being continuous transformations, a theorem from (Hocking, Young, 1961).
A6. Transformation TU*I with variable space-like domain dw and singularity w = w0
Transformation TU*[w] = (1/w) is similar to the TU*[t^^] linear in 1/t^^, it includes a singularity at w = w0 = ‘addition zero’||w, and similarly for ∆w = ∆w0 ~ w0, valid in one moment time description and time interval description, a property for w and dw not necessarily mentioned in the following. Write domain dw = [w0, w] with the series dw = [w, w/2] + Σ(z=2, Z) [w/z, w/(z+1)], which for Z infinite reduces to domain dw = [w, w/2] + [w/2, w0] = [w0, w]. For Z finite dw = [w/2, w] + [w/(Z + 1), w/2] = [w/(Z + 1), w], and singularity w = w0 is avoided. This is different from the approach for domain dt and singularity t0.
A7. Inter-dependence of the parametrisation for Pi with variable domain limits
Inter-dependence of w and tlim^^ is indicated with new independent parameters w(r1) and tlim(r2) with r2 = tlim^^(r2)/tl^^ defined in par. B4 related through parameter r. Both new parameters depend on r, the independent parameter for domain dw(r1) x dt(r2). For any TU*[∆w] the Taylor series is approximated with the terms linear in ∆wi, valid in the time interval description with ∆w and ∆wi, and due to this can be inferred to be valid for the one moment time description with w and dw from correspondence ∆w ~ w.
There is w(r1) = 1/r1. w, with specific value TU*I*[w(r1)] = w(r1) and TU*I*[tlim(r2)] = TU*I*[r2. tl] = r2. tl. Recall, for dt, multiplication follows par. B12(A3) with alternative definitions for finite t^^ from dt(finite) = [t0^^, tlim^^] and for infinite t^^ from dt(infinite) = [tlim^^, tl^^].
Surface part Qi = Pi[N, w, tlim^^], with w = w(r1) and tlim^^ = tlim^^(r2). The dw and dt are separate domains, domains follows outer products, measures of domains follow multiplication.
B20 dTU*I*[dQi] = dTU*[( [w(r1), w(r1)/2] + [w(r1)/2, w(r1)/Z+1] )] x dTU*I*[ dt(r2) ] mdTU*I*[dQi] = mdTU*[ [w(r1)/Z+1, w(r1)] ]. mdTU*I*[ dt(r2) ]
mdTU*I*[dQi] = 1/w(r1). Z. = Z. r1. 1/w. (|1/tl^^ - 1/ε(r2)|)
B21 dTU*I*[dPi] = dTU*[ ( [w, w/2] + [w/2, w/Z+1] )] x dTU*I*[ dt ]
mdTU*I*[dPi] = mdTU*[ [w/Z+1, w] ]. mdTU*I*[ dt ]
mdTU*I*[dPi] = Z. 1/w. (|1/tl^^ – 1/ε|)
Requirements are, mPi = mQi and mdTU*I*[dQi] = mdTU*I*[dPi]. It follows series parameter Z for current parameter w can be solved from the remaining parameters, and where A1 = 1/r1 = w(r1)/w, and A2 = r2 = tlim(r2)^^/tl^^ are the independent variables. Recall TU*I equals the identity transformation.
From one moment time equation mdTU*I*[w(r1)] = w(r2) it follows 1 – r1. 1/w(r1) = w(r2).
When r2 = tlim(r2)/tl^^, with tl^^ invariant, tlim^^(r2) is linear with r2, while w(r1). r1 = w remains invariant when w(r1) is linear with 1/r1. There is r2 = 1/(1 + ε(r2)).One can derive from the requirements one moment time eq. B22, where r1 and r2 both should approximate r, and w(r1), w(r2), and A1(r1) and A2(r2) similar, to evaluate solutions.
B22 w(r1). ( ε(r2) + A1(r1). (1 – ε(r2)) ) - A2(r2). (1 – w(r1)) = 0. t0
The parameters A1(r1) and A2(r2) are dependent on each other to avoid the singularity of TU at w = w0 and t^^ = t0^^. They can be adjusted independently with r1 and r2, however make sense only when related through r1 = r2 = r.
The solutions w(r1) and tlim^^(r2), when r1 = r2 = r, together add one extra degree of freedom from parameter r. Besides d2 parameter tlim^^(r), there is number of surface parts N, d1 parameter w(r), and transition parameter r ε(r) equivalent to parameter ε(r). Eq. B23 describes the mentioned requirements, and reduces the number of degrees of freedom with one.
For the time interval description there is to all orders of ∆w(r1), due to eq. 1, TU*I*[∆w(r1)] = M[∆t, (Σn Yn). ∆w(r1)] = M[M[∆w(r1)i, (exp[∆Gw] – 1). ∆t], M[∆w(r1)i, ∆w(r2)]] = ∆w(r2), the transformation being equal to the identity except when r1 and r2 not yet adjusted to be equal to r. The ∆Gw is the time interval generator for the current parameter ∆w set, similar to generator ∆G for the current parameter ∆t^^ set defined in par. B12(A4), within the time interval description, due to theorem 1c, par. 3.8.
B23 M[M[(exp[∆Gw] – 1), ∆w(r1)], ∆w(r2)] = M[(exp[∆Gw] – 1), w(r1). w(r2). M[∆t, ∆t] ] = ∆t
To retrieve a solution different from the trivial one, one can start with independent A1(r1) and A2(r2). One gathers the quadratic terms in A1 and A2, the linear terms cancel.
Assumed is commutativity of the current parameter set and the other parameter sets, since these are not dependent on one moment time or time interval only equilibrium time development or one moment time parameter t or time interval
∆t from the time interval set. The time interval only set is assumed non-commutative, (Hollestelle, 2020). Eq. B23 is quadratic in the current parameter domain measures.
When tlim^^ is assumed infinite, it follows, for dt(finite) = [t0^^, tlim^^], par. B12(A3), mw = ε(r) = |1/tlim^^| is a solution. This solution seems realistic for infinitesimal ε(r). The degrees of freedom do not change for surface parts Pi, with mdw x mdt invariant while parameter r varies, within eq. B23.
For dt(infinite) = [tlim^^, tl^^] there is solution mw = |tlim^^| = |t0^^| = ‘multiplication zero’||w, meaning wave propagation surface A, due to time development, does not change and develop away from the star source, valid for all ∆t, where m∆t = ‘multiplication unit’||∆t remains valid for all ∆t.
Theorem B6. The specific Lorentz transformations TS being quadratic in coordinates, and for which surface measure remains invariant, is defined in (Hollestelle, 2020), where specific TS are described to be an alternative to the usual Lorentz transformations TL, and one finds mdTU*I*[ dw x dt ] = md[ [w/(Z + 1), w] x [t0, tlim^^] ] and mdTU*I*[Pi] = mdTU*I*[Qi] = m[ dw x dt ], i. e. the domain measure remains invariant. This is the same result as theorem B7.
Theorem B7. Transformation TU*I, being equal to the identity, equals a specific Lorentz transformation TS. One moment time description identity equation mdTS*I*[dw x dt] = m[dw x dt], with tl^^ = ‘multiplication unit’||t^^ has only one solution, with mdw. mdt = mdw(r). mdtlim^^(r) = mw(r). r. mdtl^^ = w(r). r, which implies mQ, for regular sphere Q, equals w(r). r = w = ‘multiplication unit’||w, while mPu ≥ mQ = mA.
Theorem B8. For equation mdTS*I*[dw x dt] = ‘multiplication unit’||t, unlimited number of solutions for dw(r) x dt(r) are possible, different from and not equal to the trivial solution dw x dt, due to the n =2 dimensional domain definition t^^ = [tv, tw] from B12(A3). The transformation TU*I being equal to the identity transformation implies an addition to the fundamental theorem on polynomial equations, according to which at least one solution exists, possibly complex, for a n-degree polynomial, (Hocking, Young, 1961), (Arnold, 1989), where any application of TU*I increases the number of solutions, in this case with t^^ and n = 2, and the quadratic polynomial t^^ = tv. tw.
A8. Solutions P(N)u with more than two surface parts
When a solution P(N)u, with number N surface parts P(N)i, i = 1 to N > 2, is known, one can continue to define P(N+1)i from P(N)i. Parameter w(N+1) is chosen different from the known w for the P(N)i due to the disjoint property, however current parameter t^^(i) is chosen t^^(i) = t^^, the same for all surface parts P(N+1)i.
Comment B16. Solutions with N > 2 can be related to the multiple n star-source emission cloud collective from par. 3. To find an example surface P(N)u, apply parameter Z = N = n, with n the number of star sources, and N the number of surface parts, leaving out Z equal to infinity where singularity w0 remains unsolved.
Trivially the P(N = Z)i defined with dw(Z) and dt are disjoint when open, considering parameter w = w(N), for finite Z, they re-place and adjust space according with N = Z to N = Z + 1.
A9. Transformation from unit square to regular sphere and the wave propagation surface
A simple transformation TQ from unit square domain dq = q1. d1 x q2. d2 to a regular sphere, can be chosen with 2 of the 3 space-like parameters for TQ*[ dq ] the same as the parameters from dq, for dimensions d1 and d2.
There is: TQ*[ dq ] = q1’. d1 x q2’. d2 x q3’. d3, with space-like parameters q(i)’ = s. q(i), i = 1, 2, and q3’ = s. (1 - (q1)^2 - (q2)^2) )^(1/2). Transformation TS includes a scale transformation with scaling parameter s = m∆q = s. m∆t, however in par. 6. it is derived s = 1 due to conservation of energy. Transformation TQ ‘works to the right’ towards the Pi domain with current parameters w and t^^, which are assumed not to depend on one moment time t or time interval ∆t.
For current parameters w and t^^, when they are not considered one moment time equilibrium quantities, a corresponding time interval quantity can be found from t^^ ~ ∆t^^ = < t^^ >||∆t^^. ∆t^^. This is discussed in par. 1.5 and 2.7.
With transformation TQ*TU*I an example is constructed from current parameter domain dq = dw x dt for all ∆P(N)i, and the example approximation ∆Pu for wave propagation surface ∆A(∆t). The original Pi current parameter domain is dq = dw x dt = [w. 1/(Z + 1), w] x [t0, tlim], assumed similar for all Pi, to result in covering least requirement SR, mPu ≥ mA, with Pu, with scalar s = 1, the scaled regular sphere. This result is valid similarly within the time interval description, where ∆Pi current parameter domain d∆q = d∆w x d∆t^^ corresponds with dq.
Comment B17. Scaling parameter s = 1, according to m∆q = s. m∆t, not is meant s = m∆q. The time interval description measure m∆q can be defined by averaging, i. e. m∆q = m∆Q(n) = | < qi >||n |= < qi >||n, n the number of star-sources within the star source emission cloud. Another relation can be found from the wave propagation velocity, c(∆t) = M[∆q, ∆ti]. This approach is interesting considering the discussion for the theorem on averaging, par. 1.6.
Comment C. Specific Lorentz Transformation TS
Comment C1. In terms of specific Lorentz transformation TS, there is invariance TS*[∆dU] = ∆dU, where ∆dU = ∆NC. The acquired energy exists with units ∆NC = ∆Es, as it should be for a Noether charge related to the star source emission cloud cosmology, and suggests a qm interpretation for energies ∆Es or ∆Eg with units ∆NC = M[∆m1, ∆m2].
This seems to indicate how a coupling between energies can be expressed with a multiplication of densities. This can be applied to introduce other energy types, e. g. the open and non zero and zero equilibrium discussed in par. 3.
Star-Source Wave Emission, Gravitation Energy, and the Time Interval Only Set
Commutation properties for certain time related sets, i.e. the one moment time set and the time interval only set, were defined in (Hollestelle, 2024). Depending on the dimension d of the set, commutation properties define quantities within reciprocal d-pairs, for the time interval only set, being a one-dimensional set with d = 1, the d-pairs are 1-pairs or ordinary pairs. Where the number of degrees of freedom increases with d, maintaining equilibrium means a reduction of the number of degrees with 1, and depending on all quantities within the d-pair, one can define the invariant overall time interval Noether charge ∆NC. The Noether charge turns out to be equal to structure constants for the time interval only set. It is argued, because of this there exists a 1-pair of equivalent energies, meaning emission wave energy ∆Es and gravitation energy ∆Eg, with one moment time description time development each opposed to the other.
The 1-pair of time interval only commutation quantities are cn(∆t) and cn’(∆t), and the specific Lorentz transformation TS*[cn(∆t)] = cn’(∆t) = cn(∆t’) are related to invariance for cn’(∆t) = cn(∆t’). One finds an energy equivalence relation with a1 = ∆Es and a2 = ∆Eg.
C3 TS*[a1] = a2
TS*[a2] = A[a1, A[ I*||∆t[a2], D*||∆t[a2]iv] ] C4 |∆Eg – ∆Es| = | A[I*||∆t[∆Eg], D*||∆t[∆Eg]iv] |
Commutation relations assume the complexity of the time interval set. The d-pair of reciprocal quantities can be regarded similar to the d-pair of boundaries for some time interval: there is applied only one: 1-pair one moment time parameters t and only one: relevant event time interval ∆t, to derive the ‘set rule’ eqs. for the time interval only derivatives to t and ∆t respectively, (Hollestelle, 2024). These eqs. make sense with a non-zero factor Rest, for non- trivial commutation relations.
D*|t [a. ∆t1] = A [a. D*|t [∆t1], Rest(a)|t] Rest(a)|t = M [D*|t [a], ∆t]
D*||∆t [a. ∆t1] = A [a. D*||∆t [∆t1], Rest(a)||∆t] Rest(a)||∆t = M [D*||∆t [a], ∆t]