Cosmology as Sourced Scalar Kinematics
Record
Date: 2026-08-14
Status: conditional structural identification in finite kinematic space.
Scope: unconserved massless external momenta with a distinguished total momentum defect. This entry does not derive a cosmological state, vacuum prescription, FLRW dynamics, or integrated wavefunction.
Claim
Let
be symmetric Mandelstam space before imposing momentum conservation, and define the signless incidence map
Ordinary scattering kinematics is the kernel
For momenta with
and total momentum
the row sums are
Thus the failure of the scattering constraints is exactly the momentum defect:
within the momentum realization.
Moreover,
A canonical conserved extension is obtained by adjoining a closing leg
The enlarged system satisfies
but is generically weighted or massive:
Define defect coordinates
For massless ,
Hence the cosmological deformation away from scattering can be represented by the source data
or equivalently
subject to
The scattering locus is the source-free boundary
This gives the working sector relation
Evidence
The identification follows directly from
for , and
The closing-leg construction is the tautological conserved completion .
This is a retrospective ledger reconstruction from the cosmology investigation. No standalone repository checker has yet been attached to this entry.
Boundary
The following stronger statements are not established:
- is a new primitive of the scalar master;
- sourced kinematics alone determines a cosmological wavefunction;
- the closing leg is an ordinary additional massless particle;
- the zero-defect limit by itself determines a scattering/cosmology nearby-cycle functor;
- a choice of cosmological vacuum follows from .
The investigation instead demoted from an independent primitive: it is reconstructed from failure of the ordinary scattering constraints.
Integral bookkeeping requires retaining the primitive mass line . Eliminating it prematurely can introduce artificial torsion in the defect quotient.
Consequence
Cosmology can be tested as a derived sector of the same scalar kinematic carrier before introducing a second master geometry.
The next question is whether cosmological partial-energy boundaries are intrinsic valuations of the resolved Cut carrier or require additional sector-specific combinatorics.
Outcome contract
{
"claim": "Cosmological kinematics can be represented as the sourced complement of the ordinary scattering kernel: r_i = 2 p_i·Q, with scattering recovered at Q=0. The closing leg q_infinity=-Q gives a canonical conserved completion.",
"status": "conditional",
"assumptions": [
"External p_i are massless in the finite kinematic model.",
"The statement concerns kinematic carrier structure, not a full cosmological wavefunction.",
"No standalone checker has yet been attached."
],
"evidence_refs": [
"retrospective cosmology derivation",
"scalar-master kinematic framework"
],
"factorization_test": {
"source_map_identity": "analytic pass",
"closing_leg_conservation": "analytic pass",
"scattering_zero_defect_limit": "analytic pass",
"wavefunction_factorization": "not tested"
},
"counterevidence": [
"Sourced kinematics alone does not determine vacuum or period data.",
"The closing leg is generically massive or weighted."
],
"next_experiment": "Construct partial-energy divisors on the occurrence-resolved Cut carrier and test Cut compatibility without adding a new nesting primitive."
}