Changes between Version 4 and Version 5 of pNG

Timestamp:

Apr 3, 2020, 6:42:08 PM (5 years ago)

Author:

Ankit Beniwal

Comment:

Added JHEP version details.

pNG

@@ -3 +3 @@
 pseudo-Nambu-Goldstone (pNG) dark matter in a complex scalar singlet model with a softly broken global U(1) symmetry. 
 
-Reference: C. Arina, A. Beniwal, C. Degrande, J. Heisig and A. Scaffidi, ''Global fit of pseudo-Nambu-Goldstone Dark Matter'', 2019, arXiv:1912.04008.
+Reference: C. Arina, A. Beniwal, C. Degrande, J. Heisig and A. Scaffidi, ''Global fit of pseudo-Nambu-Goldstone Dark Matter'', JHEP04 (2020) 015, arXiv:1912.04008.
 
 === Model files ===
@@ -11 +11 @@
 Model Lagrangian is based on: C. Gross, O. Lebedev and T. Toma, ''Cancellation Mechanism for Dark-Matter–Nucleon Interaction'', Phys. Rev. Lett. 119 (2017) no. 19, 191801, [arXiv:1708.02253]
 
-Model files are available here:
+Model files include:
 
- * [/attachment/wiki/pNG/SM_with_pNG.fr FeynRules] model file and [/attachment/wiki/pNG/SM_with_pNG.nb Mathematica] notebook
+ * [/attachment/wiki/pNG/SM_with_pNG.fr FeynRules] file and [/attachment/wiki/pNG/SM_with_pNG.nb Mathematica] notebook
  * [/attachment/wiki/pNG/CalcHEP_files.zip CalcHEP files]
  * [/attachment/wiki/pNG/UFO_files.zip UFO files]
@@ -20 +20 @@
 === Contact details === 
 
-For reporting issues/bugs, please contact: A. Beniwal (ankit.beniwal@uclouvain.be). 
+For any issues/bugs, contact Ankit Beniwal (ankit.beniwal@uclouvain.be). 
 
 === Updates ===
 
-09/12/2019: Added arXiv number.
+03/04/2020: Added JHEP version details. [[BR]]
+09/12/2019: Added arXiv number.[[BR]]
 02/12/2019: Uploaded model files for the pNG DM.