Mack C. Atkinson
Transcript of Mack C. Atkinson
Exploring the link between finite nuclei and infinite nuclear matter
Mack C. Atkinson
TRIUMF
Progress in Ab Initio Techniques in Nuclear Physics
arXiv 2001.07231 Mack C. Atkinson TRIUMF 1 / 17
arXiv 2001.07231
Introduction
Fundamental properties of nuclear matter:
1 ρ0 ≈ 0.16 fm−3
2 E0 ≈ −16 MeV
Where do the values for ρ0 and E0 come from?
How does this relate to finite nuclei?
Claim: The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 2 / 17
Introduction
Fundamental properties of nuclear matter:1 ρ0 ≈ 0.16 fm−3
2 E0 ≈ −16 MeV
Where do the values for ρ0 and E0 come from?
How does this relate to finite nuclei?
Claim: The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 2 / 17
Introduction
Fundamental properties of nuclear matter:1 ρ0 ≈ 0.16 fm−3
2 E0 ≈ −16 MeV
Where do the values for ρ0 and E0 come from?
How does this relate to finite nuclei?
Claim: The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 2 / 17
Introduction
Fundamental properties of nuclear matter:1 ρ0 ≈ 0.16 fm−3
2 E0 ≈ −16 MeV
Where do the values for ρ0 and E0 come from?
How does this relate to finite nuclei?
Claim: The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 2 / 17
Introduction
Fundamental properties of nuclear matter:1 ρ0 ≈ 0.16 fm−3
2 E0 ≈ −16 MeV
Where do the values for ρ0 and E0 come from?
How does this relate to finite nuclei?
Claim: The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 2 / 17
Introduction
Fundamental properties of nuclear matter:1 ρ0 ≈ 0.16 fm−3
2 E0 ≈ −16 MeV
Where do the values for ρ0 and E0 come from?
How does this relate to finite nuclei?
Claim: The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 2 / 17
Introduction
Fundamental properties of nuclear matter:1 ρ0 ≈ 0.16 fm−3
2 E0 ≈ −16 MeV
Where do the values for ρ0 and E0 come from?
How does this relate to finite nuclei?
Claim: The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 2 / 17
Outline
1 More discussion of nuclear matter
2 Green’s function formalism
3 The dispersive optical model (DOM)
4 Binding energy densities and nuclear matter
arXiv 2001.07231 Mack C. Atkinson TRIUMF 3 / 17
Outline
1 More discussion of nuclear matter
2 Green’s function formalism
3 The dispersive optical model (DOM)
4 Binding energy densities and nuclear matter
arXiv 2001.07231 Mack C. Atkinson TRIUMF 3 / 17
Outline
1 More discussion of nuclear matter
2 Green’s function formalism
3 The dispersive optical model (DOM)
4 Binding energy densities and nuclear matter
arXiv 2001.07231 Mack C. Atkinson TRIUMF 3 / 17
Outline
1 More discussion of nuclear matter
2 Green’s function formalism
3 The dispersive optical model (DOM)
4 Binding energy densities and nuclear matter
arXiv 2001.07231 Mack C. Atkinson TRIUMF 3 / 17
Nuclear Saturation
Nuclear saturation is evident from nuclear charge radii: RA ∝ A1/3
Nuclear charge densities extracted from elastic electron-scattering experiments saturate inthe coreThese experiments revealed that this saturation density is ρ0 ≈ 0.16 fm−3
0
0.04
0.08
0.12
0.16
0 2 4 6 8 10
ρ0
ρ[fm
−3]
r [fm]
Matter Densities
16O40Ca48Ca58Ni
124Sn208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 4 / 17
Nuclear Saturation
Nuclear saturation is evident from nuclear charge radii: RA ∝ A1/3
Nuclear charge densities extracted from elastic electron-scattering experiments saturate inthe core
These experiments revealed that this saturation density is ρ0 ≈ 0.16 fm−3
0
0.04
0.08
0.12
0.16
0 2 4 6 8 10
ρ0
ρ[fm
−3]
r [fm]
Matter Densities
16O40Ca48Ca58Ni
124Sn208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 4 / 17
Nuclear Saturation
Nuclear saturation is evident from nuclear charge radii: RA ∝ A1/3
Nuclear charge densities extracted from elastic electron-scattering experiments saturate inthe core
These experiments revealed that this saturation density is ρ0 ≈ 0.16 fm−3
0
0.04
0.08
0.12
0.16
0 2 4 6 8 10
ρ0
ρ[fm
−3]
r [fm]
Matter Densities
16O40Ca48Ca58Ni
124Sn208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 4 / 17
Nuclear Saturation
Nuclear saturation is evident from nuclear charge radii: RA ∝ A1/3
Nuclear charge densities extracted from elastic electron-scattering experiments saturate inthe coreThese experiments revealed that this saturation density is ρ0 ≈ 0.16 fm−3
0
0.04
0.08
0.12
0.16
0 2 4 6 8 10
ρ0
ρ[fm
−3]
r [fm]
Matter Densities
16O40Ca48Ca58Ni
124Sn208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 4 / 17
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA− aSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA− aSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA− aSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA− aSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter
1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA− aSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA−XXXXaSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb
2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA− aSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA−XXXXaSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA−XXXXaSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface
3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA− aSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA−XXXXaSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA− aSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA−XXXXaSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA− aSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA−XXXXaSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA− aSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA−XXXXaSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Saturation Energy
arXiv 2001.07231 Mack C. Atkinson TRIUMF 5 / 17
BE (A,Z ) = aVA− aSA2/3 − 3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA− aSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1BE (A,Z ) = aVA−XXXXaSA
2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc− 1
2aA(A− 2Z )2A−1
BE (A,Z ) = aVA−XXXXaSA2/3 −
HH
HHHH
3
5
Z (Z − 1)
Rc−
XXXXXXXXX
1
2aA(A− 2Z )2A−1
Bethe-Weizsacker 1935
Infinite nuclear matter1 No Coulomb2 No surface3 Symmetric NM
=⇒ E0/A = aV ≈ −16 MeV
E0 is determined empirically (model dependent)
ρ0 ≈ 0.16 fm−3 is determined experimentally
E/A
[MeV
]
pp
W. H. Dickhoff, D. Van Neck MBT Exposed! (2008)
M. Baldo et al., PRC 86, 064001, (2012)
Single-Particle Propagator and the Dyson Equation
arXiv 2001.07231 Mack C. Atkinson TRIUMF 6 / 17
G`j(r , r′;E ) =
∑m
〈ΨA0 | ar`j |ΨA+1
m 〉 〈ΨA+1m | a†r ′`j |ΨA
0 〉E − (EA+1
m − EA0 ) + iη
+∑n
〈ΨA0 | a†r ′`j |ΨA−1
n 〉 〈ΨA−1n | ar`j |ΨA
0 〉E − (EA
0 − EA−1n )− iη
Poles correspond to excitation energies of (A + 1) or (A− 1) nucleus
Numerator like a transition probability to given excitation
Close connection with experimental observables
Perturbation expansion of G leads to the Dyson equation
If the irreducible self-energy (Σ∗) is known, then so is G= + Σ∗
Single-Particle Propagator and the Dyson Equation
arXiv 2001.07231 Mack C. Atkinson TRIUMF 6 / 17
G`j(r , r′;E ) =
∑m
〈ΨA0 | ar`j |ΨA+1
m 〉 〈ΨA+1m | a†r ′`j |ΨA
0 〉E − (EA+1
m − EA0 ) + iη
+∑n
〈ΨA0 | a†r ′`j |ΨA−1
n 〉 〈ΨA−1n | ar`j |ΨA
0 〉E − (EA
0 − EA−1n )− iη
Poles correspond to excitation energies of (A + 1) or (A− 1) nucleus
Numerator like a transition probability to given excitation
Close connection with experimental observables
Perturbation expansion of G leads to the Dyson equation
If the irreducible self-energy (Σ∗) is known, then so is G= + Σ∗
Single-Particle Propagator and the Dyson Equation
arXiv 2001.07231 Mack C. Atkinson TRIUMF 6 / 17
G`j(r , r′;E ) =
∑m
〈ΨA0 | ar`j |ΨA+1
m 〉 〈ΨA+1m | a†r ′`j |ΨA
0 〉E − (EA+1
m − EA0 ) + iη
+∑n
〈ΨA0 | a†r ′`j |ΨA−1
n 〉 〈ΨA−1n | ar`j |ΨA
0 〉E − (EA
0 − EA−1n )− iη
Poles correspond to excitation energies of (A + 1) or (A− 1) nucleus
Numerator like a transition probability to given excitation
Close connection with experimental observables
Perturbation expansion of G leads to the Dyson equation
If the irreducible self-energy (Σ∗) is known, then so is G= + Σ∗
Single-Particle Propagator and the Dyson Equation
arXiv 2001.07231 Mack C. Atkinson TRIUMF 6 / 17
G`j(r , r′;E ) =
∑m
〈ΨA0 | ar`j |ΨA+1
m 〉 〈ΨA+1m | a†r ′`j |ΨA
0 〉E − (EA+1
m − EA0 ) + iη
+∑n
〈ΨA0 | a†r ′`j |ΨA−1
n 〉 〈ΨA−1n | ar`j |ΨA
0 〉E − (EA
0 − EA−1n )− iη
Poles correspond to excitation energies of (A + 1) or (A− 1) nucleus
Numerator like a transition probability to given excitation
Close connection with experimental observables
Perturbation expansion of G leads to the Dyson equation
If the irreducible self-energy (Σ∗) is known, then so is G= + Σ∗
Single-Particle Propagator and the Dyson Equation
arXiv 2001.07231 Mack C. Atkinson TRIUMF 6 / 17
G`j(r , r′;E ) =
∑m
〈ΨA0 | ar`j |ΨA+1
m 〉 〈ΨA+1m | a†r ′`j |ΨA
0 〉E − (EA+1
m − EA0 ) + iη
+∑n
〈ΨA0 | a†r ′`j |ΨA−1
n 〉 〈ΨA−1n | ar`j |ΨA
0 〉E − (EA
0 − EA−1n )− iη
Poles correspond to excitation energies of (A + 1) or (A− 1) nucleus
Numerator like a transition probability to given excitation
Close connection with experimental observables
Perturbation expansion of G leads to the Dyson equation
If the irreducible self-energy (Σ∗) is known, then so is G
= + Σ∗
Single-Particle Propagator and the Dyson Equation
arXiv 2001.07231 Mack C. Atkinson TRIUMF 6 / 17
G`j(r , r′;E ) =
∑m
〈ΨA0 | ar`j |ΨA+1
m 〉 〈ΨA+1m | a†r ′`j |ΨA
0 〉E − (EA+1
m − EA0 ) + iη
+∑n
〈ΨA0 | a†r ′`j |ΨA−1
n 〉 〈ΨA−1n | ar`j |ΨA
0 〉E − (EA
0 − EA−1n )− iη
Poles correspond to excitation energies of (A + 1) or (A− 1) nucleus
Numerator like a transition probability to given excitation
Close connection with experimental observables
Perturbation expansion of G leads to the Dyson equation
If the irreducible self-energy (Σ∗) is known, then so is G= + Σ∗
The Dispersive Optical Model (DOM)
Irreducible self-energy at positive energies corresponds to an optical potential
Use same functional form as standard optical potentials to parametrize self-energy
Σ∗(r , r ′;E ) is explicitly nonlocal
Dispersion relation connects to negative energies
Dispersive Correction
ReΣ`j(r , r′;E ) = ReΣ`j(r , r
′; εF )− 1
π(εF − E )P
∫ ∞ε+T
dE ′ImΣ`j(r , r′;E ′)[
1
E − E ′− 1
εF − E ′]
+1
π(εF − E )P
∫ ε−T
−∞dE ′ImΣ`j(r , r
′;E ′)[1
E − E ′− 1
εF − E ′]
This constraint ensures bound and scattering quantities are simultaneously described
arXiv 2001.07231 Mack C. Atkinson TRIUMF 7 / 17
The Dispersive Optical Model (DOM)
Irreducible self-energy at positive energies corresponds to an optical potential
Use same functional form as standard optical potentials to parametrize self-energy
Σ∗(r , r ′;E ) is explicitly nonlocal
Dispersion relation connects to negative energies
Dispersive Correction
ReΣ`j(r , r′;E ) = ReΣ`j(r , r
′; εF )− 1
π(εF − E )P
∫ ∞ε+T
dE ′ImΣ`j(r , r′;E ′)[
1
E − E ′− 1
εF − E ′]
+1
π(εF − E )P
∫ ε−T
−∞dE ′ImΣ`j(r , r
′;E ′)[1
E − E ′− 1
εF − E ′]
This constraint ensures bound and scattering quantities are simultaneously described
arXiv 2001.07231 Mack C. Atkinson TRIUMF 7 / 17
The Dispersive Optical Model (DOM)
Irreducible self-energy at positive energies corresponds to an optical potential
Use same functional form as standard optical potentials to parametrize self-energy
Σ∗(r , r ′;E ) is explicitly nonlocal
Dispersion relation connects to negative energies
Dispersive Correction
ReΣ`j(r , r′;E ) = ReΣ`j(r , r
′; εF )− 1
π(εF − E )P
∫ ∞ε+T
dE ′ImΣ`j(r , r′;E ′)[
1
E − E ′− 1
εF − E ′]
+1
π(εF − E )P
∫ ε−T
−∞dE ′ImΣ`j(r , r
′;E ′)[1
E − E ′− 1
εF − E ′]
This constraint ensures bound and scattering quantities are simultaneously described
arXiv 2001.07231 Mack C. Atkinson TRIUMF 7 / 17
The Dispersive Optical Model (DOM)
Irreducible self-energy at positive energies corresponds to an optical potential
Use same functional form as standard optical potentials to parametrize self-energy
Σ∗(r , r ′;E ) is explicitly nonlocal
Dispersion relation connects to negative energies
Dispersive Correction
ReΣ`j(r , r′;E ) = ReΣ`j(r , r
′; εF )− 1
π(εF − E )P
∫ ∞ε+T
dE ′ImΣ`j(r , r′;E ′)[
1
E − E ′− 1
εF − E ′]
+1
π(εF − E )P
∫ ε−T
−∞dE ′ImΣ`j(r , r
′;E ′)[1
E − E ′− 1
εF − E ′]
This constraint ensures bound and scattering quantities are simultaneously described
arXiv 2001.07231 Mack C. Atkinson TRIUMF 7 / 17
The Dispersive Optical Model (DOM)
Irreducible self-energy at positive energies corresponds to an optical potential
Use same functional form as standard optical potentials to parametrize self-energy
Σ∗(r , r ′;E ) is explicitly nonlocal
Dispersion relation connects to negative energies
Dispersive Correction
ReΣ`j(r , r′;E ) = ReΣ`j(r , r
′; εF )− 1
π(εF − E )P
∫ ∞ε+T
dE ′ImΣ`j(r , r′;E ′)[
1
E − E ′− 1
εF − E ′]
+1
π(εF − E )P
∫ ε−T
−∞dE ′ImΣ`j(r , r
′;E ′)[1
E − E ′− 1
εF − E ′]
This constraint ensures bound and scattering quantities are simultaneously described
arXiv 2001.07231 Mack C. Atkinson TRIUMF 7 / 17
The Dispersive Optical Model (DOM)
Irreducible self-energy at positive energies corresponds to an optical potential
Use same functional form as standard optical potentials to parametrize self-energy
Σ∗(r , r ′;E ) is explicitly nonlocal
Dispersion relation connects to negative energies
Dispersive Correction
ReΣ`j(r , r′;E ) = ReΣ`j(r , r
′; εF )− 1
π(εF − E )P
∫ ∞ε+T
dE ′ImΣ`j(r , r′;E ′)[
1
E − E ′− 1
εF − E ′]
+1
π(εF − E )P
∫ ε−T
−∞dE ′ImΣ`j(r , r
′;E ′)[1
E − E ′− 1
εF − E ′]
This constraint ensures bound and scattering quantities are simultaneously described
arXiv 2001.07231 Mack C. Atkinson TRIUMF 7 / 17
Fitting the Self-energy (40Ca)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 8 / 17
Parameters of self-energy varied to minimize χ2
Reproducing the data means self-energy is found
100
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+40Ca
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
n+40Ca
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+40Ca
0
5
10
15
20
25
0 30 60 90 120 150 180
A
n+40Ca
θc.m. [deg] θc.m. [deg]
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0 1 2 3 4 5 6 7 8
ρ[e·fm
-3]
r [fm]
ExperimentDOM
0
200
400
600
800
0 50 100 150 200
p+40Ca
σ[m
b]
Elab [MeV]
05001000150020002500300035004000
0 50 100 150 200
n+40Ca
σ[m
b]
Elab [MeV]
σtotσreact
Data: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
Fitting the Self-energy (40Ca)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 8 / 17
Parameters of self-energy varied to minimize χ2
Reproducing the data means self-energy is found
100
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+40Ca
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
n+40Ca
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+40Ca
0
5
10
15
20
25
0 30 60 90 120 150 180
A
n+40Ca
θc.m. [deg] θc.m. [deg]
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0 1 2 3 4 5 6 7 8
ρ[e·fm
-3]
r [fm]
ExperimentDOM
0
200
400
600
800
0 50 100 150 200
p+40Ca
σ[m
b]
Elab [MeV]
05001000150020002500300035004000
0 50 100 150 200
n+40Ca
σ[m
b]
Elab [MeV]
σtotσreact
Data: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
Fitting the Self-energy (40Ca)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 8 / 17
Parameters of self-energy varied to minimize χ2
Reproducing the data means self-energy is found
100
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+40Ca
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
n+40Ca
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+40Ca
0
5
10
15
20
25
0 30 60 90 120 150 180
A
n+40Ca
θc.m. [deg] θc.m. [deg]
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0 1 2 3 4 5 6 7 8
ρ[e·fm
-3]
r [fm]
ExperimentDOM
0
200
400
600
800
0 50 100 150 200
p+40Ca
σ[m
b]
Elab [MeV]
05001000150020002500300035004000
0 50 100 150 200
n+40Ca
σ[m
b]
Elab [MeV]
σtotσreact
Data: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
Fitting the Self-energy (40Ca)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 8 / 17
Parameters of self-energy varied to minimize χ2
Reproducing the data means self-energy is found
100
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+40Ca
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
n+40Ca
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+40Ca
0
5
10
15
20
25
0 30 60 90 120 150 180
A
n+40Ca
θc.m. [deg] θc.m. [deg]
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0 1 2 3 4 5 6 7 8
ρ[e·fm
-3]
r [fm]
ExperimentDOM
0
200
400
600
800
0 50 100 150 200
p+40Ca
σ[m
b]
Elab [MeV]
05001000150020002500300035004000
0 50 100 150 200
n+40Ca
σ[m
b]
Elab [MeV]
σtotσreact
Data: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
Fitting the Self-energy (40Ca)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 8 / 17
Parameters of self-energy varied to minimize χ2
Reproducing the data means self-energy is found
100
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+40Ca
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
n+40Ca
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+40Ca
0
5
10
15
20
25
0 30 60 90 120 150 180
A
n+40Ca
θc.m. [deg] θc.m. [deg]
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0 1 2 3 4 5 6 7 8
ρ[e·fm
-3]
r [fm]
ExperimentDOM
0
200
400
600
800
0 50 100 150 200
p+40Ca
σ[m
b]
Elab [MeV]
05001000150020002500300035004000
0 50 100 150 200
n+40Ca
σ[m
b]
Elab [MeV]
σtotσreact
Data: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
Fitting the Self-energy (40Ca)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 8 / 17
Parameters of self-energy varied to minimize χ2
Reproducing the data means self-energy is found
100
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+40Ca
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
n+40Ca
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+40Ca
0
5
10
15
20
25
0 30 60 90 120 150 180
A
n+40Ca
θc.m. [deg] θc.m. [deg]
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0 1 2 3 4 5 6 7 8
ρ[e·fm
-3]
r [fm]
ExperimentDOM
0
200
400
600
800
0 50 100 150 200
p+40Ca
σ[m
b]
Elab [MeV]
05001000150020002500300035004000
0 50 100 150 200
n+40Ca
σ[m
b]
Elab [MeV]
σtotσreact
Data: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
Fitting the Self-energy (48Ca)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 9 / 17
Parameters of self-energy varied to minimize χ2
Reproducing the data means self-energy is found
100
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+48Ca
100
105
1010
1015
1020
1025
1030
0 30 60 90 120 150 180
n+48Ca
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+48Ca
θc.m. [deg]
−0.01
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0 1 2 3 4 5 6 7 8
ρ[e
fm-3]
r [fm]
ExperimentDOM
0
200
400
600
800
1000
0 50 100 150 200
p+48Ca
σ[m
b]
Elab [MeV]
500100015002000250030003500400045005000
0 50 100 150 200
n+48Ca
σ[m
b]
Elab [MeV]
σtot
Data: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
Fitting the Self-energy (208Pb)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 10 / 17
Parameters of self-energy varied to minimize χ2
Reproducing the data means self-energy is found
100
105
1010
1015
1020
1025
1030
1035
1040
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+208Pb
100
1010
1020
1030
1040
1050
0 30 60 90 120 150 180
n+208Pb
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
30
35
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+208Pb
0
5
10
15
20
25
0 30 60 90 120 150 180
A
n+208Pb
θc.m. [deg] θc.m. [deg]
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0 2 4 6 8 10
ρ[e
fm-3]
r [fm]
ExperimentDOM
0200400600800
1000120014001600180020002200
0 50 100 150 200
p+208Pb
σ[m
b]
Elab [MeV]
2000300040005000600070008000900010000
0 50 100 150 200
n+208Pb
σ[m
b]
Elab [MeV]
σtot
Data: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
Fitting the Self-energy (12C)
arXiv 2001.07231 Mack C. Atkinson TRIUMF 11 / 17
Parameters of self-energy varied to minimize χ2
DOM fit of 12C can be compared with ab-initioresults
100
1010
1020
1030
1040
1050
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
dσ/d
Ω[m
b/sr
]
p+12C
100
1010
1020
1030
1040
1050
0 30 60 90 120 150 180
n+12C
θc.m. [deg] θc.m. [deg]
0
5
10
15
20
25
30
35
40
45
0 30 60 90 120 150 180
Elab >100100>Elab >4040>Elab >2020>Elab >10
A
p+12C
0
5
10
15
20
25
0 30 60 90 120 150 180
A
n+12C
θc.m. [deg] θc.m. [deg]
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0 1 2 3 4 5 6
ρ[e
fm-3]
r [fm]
ExperimentDOM
0
200
400
600
0 50 100 150 200
p+12C
σ[m
b]
Elab [MeV]
200400600800100012001400160018002000
0 50 100 150 200
n+12C
σ[m
b]
Elab [MeV]
σtot
Data in DOM fit: J.M. Mueller et al. Phys. Rev. C, 83 064605, 2011
DOM Binding Energy Density
arXiv 2001.07231 Mack C. Atkinson TRIUMF 12 / 17
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
ρ2ρnTEV
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
CD-BonnAV18N3LO
Shape of E(r) is consistent with NM calculations
Core of nucleus is NM-like (ρ ≈ ρ0)
Core of nucleus minimally contributes to EA0
=⇒ NM is not well-constrained by EA0
EA0 =
1
2
∫d3r
∫d3r ′
[〈r |T |r ′〉 〈r ′|ρ|r〉+ δ3(r − r ′)
∫ ε−f
−∞dEESh(r ;E )
]= 4π
∫ ∞0
drr2E(r)p
N Z DOM EA0 Exp. EA
012C 5.80 5.90 -93.5 -92.2
40Ca 19.9 19.8 -340 -34248Ca 27.9 19.9 -418 -416
208Pb 126 81.7 -1629 -1637
Nuclear matter points: A. Rios et al., PRC 89, 044303, (2014)
DOM Binding Energy Density
arXiv 2001.07231 Mack C. Atkinson TRIUMF 12 / 17
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
ρ2ρnTEV
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
CD-BonnAV18N3LO
Shape of E(r) is consistent with NM calculations
Core of nucleus is NM-like (ρ ≈ ρ0)
Core of nucleus minimally contributes to EA0
=⇒ NM is not well-constrained by EA0
EA0 =
1
2
∫d3r
∫d3r ′
[〈r |T |r ′〉 〈r ′|ρ|r〉+ δ3(r − r ′)
∫ ε−f
−∞dEESh(r ;E )
]= 4π
∫ ∞0
drr2E(r)p
N Z DOM EA0 Exp. EA
012C 5.80 5.90 -93.5 -92.2
40Ca 19.9 19.8 -340 -34248Ca 27.9 19.9 -418 -416
208Pb 126 81.7 -1629 -1637
Nuclear matter points: A. Rios et al., PRC 89, 044303, (2014)
DOM Binding Energy Density
arXiv 2001.07231 Mack C. Atkinson TRIUMF 12 / 17
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
ρ2ρnTEV
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
CD-BonnAV18N3LO
Shape of E(r) is consistent with NM calculations
Core of nucleus is NM-like (ρ ≈ ρ0)
Core of nucleus minimally contributes to EA0
=⇒ NM is not well-constrained by EA0
EA0 =
1
2
∫d3r
∫d3r ′
[〈r |T |r ′〉 〈r ′|ρ|r〉+ δ3(r − r ′)
∫ ε−f
−∞dEESh(r ;E )
]= 4π
∫ ∞0
drr2E(r)
p
N Z DOM EA0 Exp. EA
012C 5.80 5.90 -93.5 -92.2
40Ca 19.9 19.8 -340 -34248Ca 27.9 19.9 -418 -416
208Pb 126 81.7 -1629 -1637
Nuclear matter points: A. Rios et al., PRC 89, 044303, (2014)
DOM Binding Energy Density
arXiv 2001.07231 Mack C. Atkinson TRIUMF 12 / 17
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
ρ2ρnTEV
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
CD-BonnAV18N3LO
Shape of E(r) is consistent with NM calculations
Core of nucleus is NM-like (ρ ≈ ρ0)
Core of nucleus minimally contributes to EA0
=⇒ NM is not well-constrained by EA0
EA0 =
1
2
∫d3r
∫d3r ′
[〈r |T |r ′〉 〈r ′|ρ|r〉+ δ3(r − r ′)
∫ ε−f
−∞dEESh(r ;E )
]= 4π
∫ ∞0
drr2E(r)
p
N Z DOM EA0 Exp. EA
012C 5.80 5.90 -93.5 -92.2
40Ca 19.9 19.8 -340 -34248Ca 27.9 19.9 -418 -416
208Pb 126 81.7 -1629 -1637
Nuclear matter points: A. Rios et al., PRC 89, 044303, (2014)
DOM Binding Energy Density
arXiv 2001.07231 Mack C. Atkinson TRIUMF 12 / 17
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
ρ2ρnTEV
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
CD-BonnAV18N3LO
Shape of E(r) is consistent with NM calculations
Core of nucleus is NM-like (ρ ≈ ρ0)
Core of nucleus minimally contributes to EA0
=⇒ NM is not well-constrained by EA0
EA0 =
1
2
∫d3r
∫d3r ′
[〈r |T |r ′〉 〈r ′|ρ|r〉+ δ3(r − r ′)
∫ ε−f
−∞dEESh(r ;E )
]= 4π
∫ ∞0
drr2E(r)
p
N Z DOM EA0 Exp. EA
012C 5.80 5.90 -93.5 -92.2
40Ca 19.9 19.8 -340 -34248Ca 27.9 19.9 -418 -416
208Pb 126 81.7 -1629 -1637
Nuclear matter points: A. Rios et al., PRC 89, 044303, (2014)
DOM Binding Energy Density
arXiv 2001.07231 Mack C. Atkinson TRIUMF 12 / 17
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
ρ2ρnTEV
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
CD-BonnAV18N3LO
Shape of E(r) is consistent with NM calculations
Core of nucleus is NM-like (ρ ≈ ρ0)
Core of nucleus minimally contributes to EA0
=⇒ NM is not well-constrained by EA0
EA0 =
1
2
∫d3r
∫d3r ′
[〈r |T |r ′〉 〈r ′|ρ|r〉+ δ3(r − r ′)
∫ ε−f
−∞dEESh(r ;E )
]= 4π
∫ ∞0
drr2E(r)
p
N Z DOM EA0 Exp. EA
012C 5.80 5.90 -93.5 -92.2
40Ca 19.9 19.8 -340 -34248Ca 27.9 19.9 -418 -416
208Pb 126 81.7 -1629 -1637
Nuclear matter points: A. Rios et al., PRC 89, 044303, (2014)
DOM Binding Energy Density
arXiv 2001.07231 Mack C. Atkinson TRIUMF 12 / 17
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
ρ2ρnTEV
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
CD-BonnAV18N3LO
Shape of E(r) is consistent with NM calculations
Core of nucleus is NM-like (ρ ≈ ρ0)
Core of nucleus minimally contributes to EA0
=⇒ NM is not well-constrained by EA0
EA0 =
1
2
∫d3r
∫d3r ′
[〈r |T |r ′〉 〈r ′|ρ|r〉+ δ3(r − r ′)
∫ ε−f
−∞dEESh(r ;E )
]= 4π
∫ ∞0
drr2E(r)
p
N Z DOM EA0 Exp. EA
012C 5.80 5.90 -93.5 -92.2
40Ca 19.9 19.8 -340 -34248Ca 27.9 19.9 -418 -416
208Pb 126 81.7 -1629 -1637
Nuclear matter points: A. Rios et al., PRC 89, 044303, (2014)
DOM Binding Energy Density
arXiv 2001.07231 Mack C. Atkinson TRIUMF 12 / 17
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
−15
−10
−5
0
5
10
15
0 1 2 3 4 5 6 7 8
40Ca
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
ρ2ρnTEV
4πr2E/A
[MeV·fm
−3]
4πr2ρ
[fm−3]
r [fm]
CD-BonnAV18N3LO
Shape of E(r) is consistent with NM calculations
Core of nucleus is NM-like (ρ ≈ ρ0)
Core of nucleus minimally contributes to EA0
=⇒ NM is not well-constrained by EA0
EA0 =
1
2
∫d3r
∫d3r ′
[〈r |T |r ′〉 〈r ′|ρ|r〉+ δ3(r − r ′)
∫ ε−f
−∞dEESh(r ;E )
]= 4π
∫ ∞0
drr2E(r)
p
N Z DOM EA0 Exp. EA
012C 5.80 5.90 -93.5 -92.2
40Ca 19.9 19.8 -340 -34248Ca 27.9 19.9 -418 -416
208Pb 126 81.7 -1629 -1637
Nuclear matter points: A. Rios et al., PRC 89, 044303, (2014)
3N Contribution
arXiv 2001.07231 Mack C. Atkinson TRIUMF 13 / 17
Energy sum-rule used in DOM assumes no 3-body force
Variational Monte Carlo (VMC) calculations show small 3N contribution
Verifies that the lack of a 3N force in DOM calculations does not affect conclusions
−25−20−15−10−505
10152025
0 1 2 3 4 5
12C
4πr2E/A
[MeV·fm
−3]
r [fm]
VMC using AV18+UX
ρETVU
−1
0
1
0 1 2 3 4 5
r [fm]
3N Potential Densities
Urbana-XNV3-Ib*NV3-Ia*
NV3-IIb*NV3-IIa*
−4
−3
−2
−1
0
1
0 1 2 3 4 5
r [fm]
Energy Densities
Chiral Interactions: M. Piarulli et al., PRL 120, 052503, (2018)
3N Contribution
arXiv 2001.07231 Mack C. Atkinson TRIUMF 13 / 17
Energy sum-rule used in DOM assumes no 3-body force
Variational Monte Carlo (VMC) calculations show small 3N contribution
Verifies that the lack of a 3N force in DOM calculations does not affect conclusions
−25−20−15−10−505
10152025
0 1 2 3 4 5
12C
4πr2E/A
[MeV·fm
−3]
r [fm]
VMC using AV18+UX
ρETVU
−1
0
1
0 1 2 3 4 5
r [fm]
3N Potential Densities
Urbana-XNV3-Ib*NV3-Ia*
NV3-IIb*NV3-IIa*
−4
−3
−2
−1
0
1
0 1 2 3 4 5
r [fm]
Energy Densities
Chiral Interactions: M. Piarulli et al., PRL 120, 052503, (2018)
3N Contribution
arXiv 2001.07231 Mack C. Atkinson TRIUMF 13 / 17
Energy sum-rule used in DOM assumes no 3-body force
Variational Monte Carlo (VMC) calculations show small 3N contribution
Verifies that the lack of a 3N force in DOM calculations does not affect conclusions
−25−20−15−10−505
10152025
0 1 2 3 4 5
12C
4πr2E/A
[MeV·fm
−3]
r [fm]
VMC using AV18+UX
ρETVU
−1
0
1
0 1 2 3 4 5
r [fm]
3N Potential Densities
Urbana-XNV3-Ib*NV3-Ia*
NV3-IIb*NV3-IIa*
−4
−3
−2
−1
0
1
0 1 2 3 4 5
r [fm]
Energy Densities
Chiral Interactions: M. Piarulli et al., PRL 120, 052503, (2018)
3N Contribution
arXiv 2001.07231 Mack C. Atkinson TRIUMF 13 / 17
Energy sum-rule used in DOM assumes no 3-body force
Variational Monte Carlo (VMC) calculations show small 3N contribution
Verifies that the lack of a 3N force in DOM calculations does not affect conclusions
−25−20−15−10−505
10152025
0 1 2 3 4 5
12C
4πr2E/A
[MeV·fm
−3]
r [fm]
VMC using AV18+UX
ρETVU
−1
0
1
0 1 2 3 4 5
r [fm]
3N Potential Densities
Urbana-XNV3-Ib*NV3-Ia*
NV3-IIb*NV3-IIa*
−4
−3
−2
−1
0
1
0 1 2 3 4 5
r [fm]
Energy Densities
Chiral Interactions: M. Piarulli et al., PRL 120, 052503, (2018)
3N Contribution
arXiv 2001.07231 Mack C. Atkinson TRIUMF 13 / 17
Energy sum-rule used in DOM assumes no 3-body force
Variational Monte Carlo (VMC) calculations show small 3N contribution
Verifies that the lack of a 3N force in DOM calculations does not affect conclusions
−25−20−15−10−505
10152025
0 1 2 3 4 5
12C
4πr2E/A
[MeV·fm
−3]
r [fm]
VMC using AV18+UX
ρETVU
−1
0
1
0 1 2 3 4 5
r [fm]
3N Potential Densities
Urbana-XNV3-Ib*NV3-Ia*
NV3-IIb*NV3-IIa*
−4
−3
−2
−1
0
1
0 1 2 3 4 5
r [fm]
Energy Densities
Chiral Interactions: M. Piarulli et al., PRL 120, 052503, (2018)
Energy in 208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 14 / 17
Large core of 208Pb makes it ideal to study
Must remove effect of Coulomb
Account for asymmetry:BE = aVA− 1
2aA(A− 2Z )2A−1
Energy does not match canonical value −18
−16
−14
−12
−10
−8
0 1 2 3 4 5 6
208Pb
E/A
[MeV
]
r [fm]
DOMAV18
EA0 =
EA0
A
∫d3rρ(r) =
∫d3rE(r) =⇒ E(r) =
(EA
0
A
)ρ(r) =⇒ E (r) ≈ A
E(r)
ρ(r)
Energy in 208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 14 / 17
Large core of 208Pb makes it ideal to study
Must remove effect of Coulomb
Account for asymmetry:BE = aVA− 1
2aA(A− 2Z )2A−1
Energy does not match canonical value
−18
−16
−14
−12
−10
−8
0 1 2 3 4 5 6
208Pb
E/A
[MeV
]r [fm]
DOMAV18
EA0 =
EA0
A
∫d3rρ(r) =
∫d3rE(r) =⇒ E(r) =
(EA
0
A
)ρ(r) =⇒ E (r) ≈ A
E(r)
ρ(r)
Energy in 208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 14 / 17
Large core of 208Pb makes it ideal to study
Must remove effect of Coulomb
Account for asymmetry:BE = aVA− 1
2aA(A− 2Z )2A−1
Energy does not match canonical value
−18
−16
−14
−12
−10
−8
0 1 2 3 4 5 6
208Pb
E/A
[MeV
]r [fm]
DOMAV18
EA0 =
EA0
A
∫d3rρ(r) =
∫d3rE(r) =⇒ E(r) =
(EA
0
A
)ρ(r) =⇒ E (r) ≈ A
E(r)
ρ(r)
Energy in 208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 14 / 17
Large core of 208Pb makes it ideal to study
Must remove effect of Coulomb
Account for asymmetry:BE = aVA− 1
2aA(A− 2Z )2A−1
Energy does not match canonical value
−18
−16
−14
−12
−10
−8
0 1 2 3 4 5 6
208Pb
E/A
[MeV
]r [fm]
DOMAV18
EA0 =
EA0
A
∫d3rρ(r) =
∫d3rE(r) =⇒ E(r) =
(EA
0
A
)ρ(r) =⇒ E (r) ≈ A
E(r)
ρ(r)
Energy in 208Pb
arXiv 2001.07231 Mack C. Atkinson TRIUMF 14 / 17
Large core of 208Pb makes it ideal to study
Must remove effect of Coulomb
Account for asymmetry:BE = aVA− 1
2aA(A− 2Z )2A−1
Energy does not match canonical value −18
−16
−14
−12
−10
−8
0 1 2 3 4 5 6
208Pb
E/A
[MeV
]r [fm]
DOMAV18
EA0 =
EA0
A
∫d3rρ(r) =
∫d3rE(r) =⇒ E(r) =
(EA
0
A
)ρ(r) =⇒ E (r) ≈ A
E(r)
ρ(r)
Energy in the Interior
arXiv 2001.07231 Mack C. Atkinson TRIUMF 15 / 17
Energy of each nucleus consistently above -16 MeV
Consistent with SCGF calculation in NM
−16
−14
−12
−10
−8
−6
0 0.2 0.4 0.6 0.8 1 1.2 1.4
−16
−14
−12
−10
−8
−6
0 0.2 0.4 0.6 0.8 1 1.2 1.4
E/A
[MeV
]
r [fm]
12C40Ca48Ca
E/A
[MeV
]
r [fm]
208PbAV18
E/A
[MeV
]
pp
M. Baldo et al., PRC 86, 064001, (2012)
Energy in the Interior
arXiv 2001.07231 Mack C. Atkinson TRIUMF 15 / 17
Energy of each nucleus consistently above -16 MeV
Consistent with SCGF calculation in NM
−16
−14
−12
−10
−8
−6
0 0.2 0.4 0.6 0.8 1 1.2 1.4
−16
−14
−12
−10
−8
−6
0 0.2 0.4 0.6 0.8 1 1.2 1.4
E/A
[MeV
]
r [fm]
12C40Ca48Ca
E/A
[MeV
]
r [fm]
208PbAV18
E/A
[MeV
]
pp
M. Baldo et al., PRC 86, 064001, (2012)
Energy in the Interior
arXiv 2001.07231 Mack C. Atkinson TRIUMF 15 / 17
Energy of each nucleus consistently above -16 MeV
Consistent with SCGF calculation in NM
−16
−14
−12
−10
−8
−6
0 0.2 0.4 0.6 0.8 1 1.2 1.4
−16
−14
−12
−10
−8
−6
0 0.2 0.4 0.6 0.8 1 1.2 1.4
E/A
[MeV
]
r [fm]
12C40Ca48Ca
E/A
[MeV
]
r [fm]
208PbAV18
E/A
[MeV
]
pp
M. Baldo et al., PRC 86, 064001, (2012)
Summary
Canonical value of saturation energy is determined empirically from the mass formula
Minimal contribution to the binding energy from the core of the nucleus=⇒ Empirical mass formula is not a great constraint for NM
Results are consistent with SCGF calculation of NM using AV18
The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 16 / 17
Summary
Canonical value of saturation energy is determined empirically from the mass formula
Minimal contribution to the binding energy from the core of the nucleus
=⇒ Empirical mass formula is not a great constraint for NM
Results are consistent with SCGF calculation of NM using AV18
The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 16 / 17
Summary
Canonical value of saturation energy is determined empirically from the mass formula
Minimal contribution to the binding energy from the core of the nucleus=⇒ Empirical mass formula is not a great constraint for NM
Results are consistent with SCGF calculation of NM using AV18
The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 16 / 17
Summary
Canonical value of saturation energy is determined empirically from the mass formula
Minimal contribution to the binding energy from the core of the nucleus=⇒ Empirical mass formula is not a great constraint for NM
Results are consistent with SCGF calculation of NM using AV18
The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 16 / 17
Summary
Canonical value of saturation energy is determined empirically from the mass formula
Minimal contribution to the binding energy from the core of the nucleus=⇒ Empirical mass formula is not a great constraint for NM
Results are consistent with SCGF calculation of NM using AV18
The value of E0 is not necessarily -16 MeV
arXiv 2001.07231 Mack C. Atkinson TRIUMF 16 / 17
Thanks
arXiv 2001.07231 Mack C. Atkinson TRIUMF 17 / 17
Willem Dickhoff
Maria Piarulli
Robert Charity
Hossein Mahzoon
Lee Sobotka
Cole Pruitt
Natalie Calleya
Bob Wiringa
Arnau Rios