Measurement of key resonance states for the 40P(p,g)31S reaction rate, and the production of intermediate-mass elements in nova explosions

Constraining the $^{30}$P$(p; γ)^{31}$S reaction rate in one novae via the weak, low-energy, β-delayed proton decay of $^{31}$Cl

Budner, T.
Friedman, M.
Wrede, C.
Brown, B.A.
José, J.
Pérez-Loureiro, D.
Sun, L.J.
Surbrook, J.
Ayyad, Y.
Bardayan, D.W.
Chae, K.
Chen, A.A.
Chipps, K.A.
Cortesi, M.
Glassman, B.
Hall, M.R.
Janasik, M.
Liang, J.
O'Malley, P.
Pollacco, E.
Psaltis, A.
Stomps, J.
Wheeler, T.

January 2022

International audienceThe P30(p,γ)S31 reaction plays an important role in understanding the nucleosy...

Study of key resonances in the $^{30}$P(p,γ)$^{31}$S reaction in classical novae

Meyer, A.
De Séréville, N.
Hammache, F.
Adsley, P.
Assié, M.
Beaumel, D.
Delafosse, C.
Flavigny, F.
Georgiadou, A.
Gottardo, A.
Grassi, L.
Guillot, J.
Barkach, T.Id
MacCormick, M.
Matea, I.
Olivier, L.
Perrot, L.
Portail, C.
Stefan, I.
Parikh, A.
Coc, A.
Kiener, J.
Tatischeff, V.
Laird, A.M.
Fox, S.P.
Hubbard, N.
Riley, J.
De Oliveira, F.
Bastin, B.
Béroff, K.
Sanchez Benitez, A.M.
Alellara, A.
Assunção, M.
Guimaraes, V.
Oulebsir, N.
D'Agata, G.

September 2017

International audienceAmong reactions with strong impact on classical novae model predictions, 30P(p...

Direct Measurement of the 21Na(p,y)22Mg Resonant Reaction Rate in Nova Nucleosynthesis

Bishop, Shawn

January 2003

An oxygen-neon nova is presently understood to be the result of a thermonuclear runaway on the surf...

Measurement of key resonance states for the 40P(p,g)31S reaction rate, and the production of intermediate-mass elements in nova explosions

Kankainen, A
Woods, P.J.
Schatz, H.
Poxon-Pearson, T
Doherty, D.T.
Bader, V.
Baugher, T.
Bazin, D.
Brown, B.A.
Browne, J.
Estrade, A.
Gade, A.
José Pont, Jordi
Kontos, A.
Langer, C.
Lotay, G.
Meisel, Z.
Montes, F.
Noji, S.
Nunes, F.
Perdikakis, G.
Pereira, J.
Recchia, F.
Redpath, T.
Stroberg, R.
Scott, M.
Seweryniak, D.
Stevens, J.
Weisshaar, D.
Wimmer, K.
Zegers, R.

May 2017

We report the first experimental constraints on spectroscopic factors and strengths of key resonance...

Measurement of key resonance states for the 30P(p, γ)31Sreaction rate, and the production of intermediate-mass elements in nova explosions

Kankainen, A
Woods, PJ
Schatz, H
Poxon-Pearson, T
Doherty, Daniel
Bader, V
Baugher, T
Bazin, D
Brown, BA
Browne, J
Estrade, A
Gade, A
José, J
Kontos, A
Langer, C
Lotay, Gavin
Meisel, Z
Montes, F
Noji, S
Nunes, F
Perdikakis, G
Pereira, J
Recchia, F
Redpath, T
Stroberg, R
Scott, M
Seweryniak, D
Stevens, J
Weisshaar, D
Zegers, R

January 2019

We report the first experimental constraints on spectroscopic factors and strengths of key resonance...

Key resonances in the 30P(p,γ)31S gateway reaction for the production of heavy elements in ONe novae.

Doherty, DT
Lotay, G
Woods, PJ
Seweryniak, D
Carpenter, MP
Chiara, CJ
David, HM
Janssens, RV
Trache, L
Zhu, S

January 2020

Material emitted as ejecta from ONe novae outbursts is observed to be rich in elements as heavy as C...

Experimental studies for explosive nuclear astrophysics

Doherty, Daniel Thomas

June 2014

In the ejecta from ONe novae outbursts nuclei up to A~40 are observed. The 30P(p,γ)31S reaction is ...

Investigating the Phosphorus-30 Proton Capture Reaction in Classical Novae

Burcher, Sean

December 2019

AbstractAccurate modeling of classical nova nucleosynthesis is fundamentally dependent on ...

Direct measurement of astrophysically important resonances in 38K( p,γ )39Ca

Christian, G
Lotay, Gavin
Ruiz, C
Akers, C
Burke, D
Catford, Wilton
Chen, A
Connolly, D
Davids, B
Fallis, J
Hager, U
Hutcheon, D
Mahl, A
Rojas, A
Sun, X

January 2019

Background: Classical novae are cataclysmic nuclear explosions occurring when a white dwarf in a bin...

Constraining the 30P(p,γ)31S reaction using 30P(d,pγ)31P with GODDESS

Ghimire, Rajesh

December 2022

The 30P(p,γ)31S reaction acts as a bottleneck for classical nova nucleosynthesis beyond A=30 in ONe ...

Level structure of 30S: Implications for the astrophysical 29P(p,γ)30S reaction rate in ONe novae and x-ray bursts

Lotay, G
Wallace, JP
Woods, PJ
Seweryniak, D
Carpenter, MP
Chiara, CJ
Doherty, DT
Janssens, RVF
Lauritsen, T
Rogers, AM
Zhu, S

January 2020

A γ-ray spectroscopy study of 30S is presented. Excitation energies have been determined with improv...

Study of key resonances in the 30P(p,γ)31S reaction in classical novae

Meyer A.
de Séréville N.
Hammache F.
Adsley P.
Assié M.
Beaumel D.
Delafosse C.
Flavigny F.
Georgiadou A.
Gottardo A.
Grassi L.
Guillot J.
Id Barkach T.
MacCormick M.
Matea I.
Olivier L.
Perrot L.
Portail C.
Stefan I.
Parikh A.
Coc A.
Kiener J.
Tatischeff V.
Laird A. M.
Fox S. P.
Hubbard N.
Riley J.
De Oliveira F.
Bastin B.
Béroff K.
Sánchez Benítez Á. M.
Alellara A.
Assunção M.
Guimaraes V.
Oulebsir N.
D’Agata G.

January 2018

Among reactions with strong impact on classical novae model predictions, 30P(p,γ)31S is one of the f...

Study of astrophysically important resonant states in 30 S using the 32S(p,t)30 S reaction

K. Setoodehnia
A.A. Chen
J. Chen
J.A. Clark
C. Deibel
D. Kahl
W.N. Lennard
P.D. Parker
C. Wrede

March 2010

A small fraction (< 1%) of presolar SiC grains is suggested to have been formed in the eje...

Study of astrophysically important resonant states in 30 S using the 32S(p,t)30 S reaction

Wrede C.
Lennard W.N.
Parker P.D.
Deibel C.
Kahl D.
Chen J.
Clark J.A.
Setoodehnia K.
Chen A.A.

March 2010

A small fraction (< 1%) of presolar SiC grains is suggested to have been formed in the ejecta of cl...

Study of astrophysically important resonant states in 30S using the 32S(p,t)30S reaction

Kiana Setoodehnia
Alan A. Chen
Jun Chen
Jason A. Clark
Catherine Deibel
David Kahl
William N
Peter D. Parker
Christopher Wrede

August 2016

Abstract. A small fraction (< 1%) of presolar SiC grains is suggested to have been formed in the ...

Constraining the $^{30}$P$(p; γ)^{31}$S reaction rate in one novae via the weak, low-energy, β-delayed proton decay of $^{31}$Cl

Budner, T.
Friedman, M.
Wrede, C.
Brown, B.A.
José, J.
Pérez-Loureiro, D.
Sun, L.J.
Surbrook, J.
Ayyad, Y.
Bardayan, D.W.
Chae, K.
Chen, A.A.
Chipps, K.A.
Cortesi, M.
Glassman, B.
Hall, M.R.
Janasik, M.
Liang, J.
O'Malley, P.
Pollacco, E.
Psaltis, A.
Stomps, J.
Wheeler, T.

January 2022

International audienceThe P30(p,γ)S31 reaction plays an important role in understanding the nucleosy...

Study of key resonances in the $^{30}$P(p,γ)$^{31}$S reaction in classical novae

Meyer, A.
De Séréville, N.
Hammache, F.
Adsley, P.
Assié, M.
Beaumel, D.
Delafosse, C.
Flavigny, F.
Georgiadou, A.
Gottardo, A.
Grassi, L.
Guillot, J.
Barkach, T.Id
MacCormick, M.
Matea, I.
Olivier, L.
Perrot, L.
Portail, C.
Stefan, I.
Parikh, A.
Coc, A.
Kiener, J.
Tatischeff, V.
Laird, A.M.
Fox, S.P.
Hubbard, N.
Riley, J.
De Oliveira, F.
Bastin, B.
Béroff, K.
Sanchez Benitez, A.M.
Alellara, A.
Assunção, M.
Guimaraes, V.
Oulebsir, N.
D'Agata, G.

September 2017

International audienceAmong reactions with strong impact on classical novae model predictions, 30P(p...

Direct Measurement of the 21Na(p,y)22Mg Resonant Reaction Rate in Nova Nucleosynthesis

Bishop, Shawn

January 2003

An oxygen-neon nova is presently understood to be the result of a thermonuclear runaway on the surf...

Measurement of key resonance states for the 40P(p,g)31S reaction rate, and the production of intermediate-mass elements in nova explosions

Kankainen, A
Woods, P.J.
Schatz, H.
Poxon-Pearson, T
Doherty, D.T.
Bader, V.
Baugher, T.
Bazin, D.
Brown, B.A.
Browne, J.
Estrade, A.
Gade, A.
José Pont, Jordi
Kontos, A.
Langer, C.
Lotay, G.
Meisel, Z.
Montes, F.
Noji, S.
Nunes, F.
Perdikakis, G.
Pereira, J.
Recchia, F.
Redpath, T.
Stroberg, R.
Scott, M.
Seweryniak, D.
Stevens, J.
Weisshaar, D.
Wimmer, K.
Zegers, R.

May 2017

We report the first experimental constraints on spectroscopic factors and strengths of key resonance...

Measurement of key resonance states for the 30P(p, γ)31Sreaction rate, and the production of intermediate-mass elements in nova explosions

Kankainen, A
Woods, PJ
Schatz, H
Poxon-Pearson, T
Doherty, Daniel
Bader, V
Baugher, T
Bazin, D
Brown, BA
Browne, J
Estrade, A
Gade, A
José, J
Kontos, A
Langer, C
Lotay, Gavin
Meisel, Z
Montes, F
Noji, S
Nunes, F
Perdikakis, G
Pereira, J
Recchia, F
Redpath, T
Stroberg, R
Scott, M
Seweryniak, D
Stevens, J
Weisshaar, D
Zegers, R

January 2019

We report the first experimental constraints on spectroscopic factors and strengths of key resonance...

Key resonances in the 30P(p,γ)31S gateway reaction for the production of heavy elements in ONe novae.

Doherty, DT
Lotay, G
Woods, PJ
Seweryniak, D
Carpenter, MP
Chiara, CJ
David, HM
Janssens, RV
Trache, L
Zhu, S

January 2020

Material emitted as ejecta from ONe novae outbursts is observed to be rich in elements as heavy as C...

Experimental studies for explosive nuclear astrophysics

Doherty, Daniel Thomas

June 2014

In the ejecta from ONe novae outbursts nuclei up to A~40 are observed. The 30P(p,γ)31S reaction is ...

Investigating the Phosphorus-30 Proton Capture Reaction in Classical Novae

Burcher, Sean

December 2019

AbstractAccurate modeling of classical nova nucleosynthesis is fundamentally dependent on ...

Direct measurement of astrophysically important resonances in 38K( p,γ )39Ca

Christian, G
Lotay, Gavin
Ruiz, C
Akers, C
Burke, D
Catford, Wilton
Chen, A
Connolly, D
Davids, B
Fallis, J
Hager, U
Hutcheon, D
Mahl, A
Rojas, A
Sun, X

January 2019

Background: Classical novae are cataclysmic nuclear explosions occurring when a white dwarf in a bin...

Constraining the 30P(p,γ)31S reaction using 30P(d,pγ)31P with GODDESS

Ghimire, Rajesh

December 2022

The 30P(p,γ)31S reaction acts as a bottleneck for classical nova nucleosynthesis beyond A=30 in ONe ...

Level structure of 30S: Implications for the astrophysical 29P(p,γ)30S reaction rate in ONe novae and x-ray bursts

Lotay, G
Wallace, JP
Woods, PJ
Seweryniak, D
Carpenter, MP
Chiara, CJ
Doherty, DT
Janssens, RVF
Lauritsen, T
Rogers, AM
Zhu, S

January 2020

A γ-ray spectroscopy study of 30S is presented. Excitation energies have been determined with improv...

Study of key resonances in the 30P(p,γ)31S reaction in classical novae

Meyer A.
de Séréville N.
Hammache F.
Adsley P.
Assié M.
Beaumel D.
Delafosse C.
Flavigny F.
Georgiadou A.
Gottardo A.
Grassi L.
Guillot J.
Id Barkach T.
MacCormick M.
Matea I.
Olivier L.
Perrot L.
Portail C.
Stefan I.
Parikh A.
Coc A.
Kiener J.
Tatischeff V.
Laird A. M.
Fox S. P.
Hubbard N.
Riley J.
De Oliveira F.
Bastin B.
Béroff K.
Sánchez Benítez Á. M.
Alellara A.
Assunção M.
Guimaraes V.
Oulebsir N.
D’Agata G.

January 2018

Among reactions with strong impact on classical novae model predictions, 30P(p,γ)31S is one of the f...

Study of astrophysically important resonant states in 30 S using the 32S(p,t)30 S reaction

K. Setoodehnia
A.A. Chen
J. Chen
J.A. Clark
C. Deibel
D. Kahl
W.N. Lennard
P.D. Parker
C. Wrede

March 2010

A small fraction (< 1%) of presolar SiC grains is suggested to have been formed in the eje...

Study of astrophysically important resonant states in 30 S using the 32S(p,t)30 S reaction

Wrede C.
Lennard W.N.
Parker P.D.
Deibel C.
Kahl D.
Chen J.
Clark J.A.
Setoodehnia K.
Chen A.A.

March 2010

A small fraction (< 1%) of presolar SiC grains is suggested to have been formed in the ejecta of cl...

Study of astrophysically important resonant states in 30S using the 32S(p,t)30S reaction

Kiana Setoodehnia
Alan A. Chen
Jun Chen
Jason A. Clark
Catherine Deibel
David Kahl
William N
Peter D. Parker
Christopher Wrede

August 2016

Abstract. A small fraction (< 1%) of presolar SiC grains is suggested to have been formed in the ...

Constraining the $^{30}$P$(p; γ)^{31}$S reaction rate in one novae via the weak, low-energy, β-delayed proton decay of $^{31}$Cl

Budner, T.
Friedman, M.
Wrede, C.
Brown, B.A.
José, J.
Pérez-Loureiro, D.
Sun, L.J.
Surbrook, J.
Ayyad, Y.
Bardayan, D.W.
Chae, K.
Chen, A.A.
Chipps, K.A.
Cortesi, M.
Glassman, B.
Hall, M.R.
Janasik, M.
Liang, J.
O'Malley, P.
Pollacco, E.
Psaltis, A.
Stomps, J.
Wheeler, T.

January 2022

International audienceThe P30(p,γ)S31 reaction plays an important role in understanding the nucleosy...

Study of key resonances in the $^{30}$P(p,γ)$^{31}$S reaction in classical novae

Meyer, A.
De Séréville, N.
Hammache, F.
Adsley, P.
Assié, M.
Beaumel, D.
Delafosse, C.
Flavigny, F.
Georgiadou, A.
Gottardo, A.
Grassi, L.
Guillot, J.
Barkach, T.Id
MacCormick, M.
Matea, I.
Olivier, L.
Perrot, L.
Portail, C.
Stefan, I.
Parikh, A.
Coc, A.
Kiener, J.
Tatischeff, V.
Laird, A.M.
Fox, S.P.
Hubbard, N.
Riley, J.
De Oliveira, F.
Bastin, B.
Béroff, K.
Sanchez Benitez, A.M.
Alellara, A.
Assunção, M.
Guimaraes, V.
Oulebsir, N.
D'Agata, G.

September 2017

International audienceAmong reactions with strong impact on classical novae model predictions, 30P(p...

Direct Measurement of the 21Na(p,y)22Mg Resonant Reaction Rate in Nova Nucleosynthesis

Bishop, Shawn

January 2003

An oxygen-neon nova is presently understood to be the result of a thermonuclear runaway on the surf...

Measurement of key resonance states for the 40P(p,g)31S reaction rate, and the production of intermediate-mass elements in nova explosions

Abstract

Extracted data

Measurement of key resonance states for the 40P(p,g)31S reaction rate, and the production of intermediate-mass elements in nova explosions

Abstract

Extracted data

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